Physics Book - User contributions [en]

Total Angular Momentum

2023-12-04T02:07:13Z

DanOConnor: /* Connectedness */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

===Computational Model for this problem===
[[File:AngularMomentumGif.gif]]

Here the angular momentum points in the negative z-hat direction because the masses are moving clockwise (both Ltrans and Lrot)

In order to update the positions of the masses in this computational model, you need to find the new position of the masses with respect to the center that it is rotating around (in this case it is the axis which we used to calculate lrot) and you need the new position of the rod that is rotating.

To calculate the new position of the masses with respect to the axis they are rotating around (Lrot), we need to find the change in angle between the last iteration and the new one, then we need to use trig.

To find the new angle we can take the old angle and add it to w * deltat

:<math> \theta_{f} = \theta_{i} + \vec{w_{2}}\times \Delta t </math>

[[File:Diag1angularmom.png]]

Now, the new position of the mass 1 is just

:<math> \vec{r_{mc2}} = <d/2(cos(\theta), d/2sin(\theta), 0)> </math>

For Mass 2, it's the same but with an angle that is 180 degrees less than theta.

Now we have to find the arrangement of the first cylinder.

:<math> \theta_{f} = \theta_{i} + \vec{w_{1}} \times \Delta t </math>

:<math> \vec{r_{cyl}} = <b(sin(\theta)), b(cos(theta)), 0> </math>

Then the positions of the two masses are just these two vectors added together.

:<math> \vec{r_{m}} = \vec{r_{cyl}} + \vec{r_{mc2}} </math>

The link to the code:
https://www.glowscript.org/#/user/danielisme18/folder/MyPrograms/program/angularMomentump1

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-04T02:02:24Z

DanOConnor: /* Computational Model for this problem */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

===Computational Model for this problem===
[[File:AngularMomentumGif.gif]]

Here the angular momentum points in the negative z-hat direction because the masses are moving clockwise (both Ltrans and Lrot)

In order to update the positions of the masses in this computational model, you need to find the new position of the masses with respect to the center that it is rotating around (in this case it is the axis which we used to calculate lrot) and you need the new position of the rod that is rotating.

To calculate the new position of the masses with respect to the axis they are rotating around (Lrot), we need to find the change in angle between the last iteration and the new one, then we need to use trig.

To find the new angle we can take the old angle and add it to w * deltat

:<math> \theta_{f} = \theta_{i} + \vec{w_{2}}\times \Delta t </math>

[[File:Diag1angularmom.png]]

Now, the new position of the mass 1 is just

:<math> \vec{r_{mc2}} = <d/2(cos(\theta), d/2sin(\theta), 0)> </math>

For Mass 2, it's the same but with an angle that is 180 degrees less than theta.

Now we have to find the arrangement of the first cylinder.

:<math> \theta_{f} = \theta_{i} + \vec{w_{1}} \times \Delta t </math>

:<math> \vec{r_{cyl}} = <b(sin(\theta)), b(cos(theta)), 0> </math>

Then the positions of the two masses are just these two vectors added together.

:<math> \vec{r_{m}} = \vec{r_{cyl}} + \vec{r_{mc2}} </math>

The link to the code:
https://www.glowscript.org/#/user/danielisme18/folder/MyPrograms/program/angularMomentump1

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-04T02:01:32Z

DanOConnor: /* Computational Model for this problem */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

===Computational Model for this problem===
[[File:AngularMomentumGif.gif]]

Here the angular momentum points in the negative z-hat direction because the masses are moving clockwise (both Ltrans and Lrot)

In order to update the positions of the masses in this computational model, you need to find the new position of the masses with respect to the center that it is rotating around (in this case it is the axis which we used to calculate lrot) and you need the new position of the rod that is rotating.

To calculate the new position of the masses with respect to the axis they are rotating around (Lrot), we need to find the change in angle between the last iteration and the new one, then we need to use trig.

To find the new angle we can take the old angle and add it to w * deltat

:<math> \theta_{f} = \theta_{i} + \vec{w_{2}}\times \Delta t </math>

[[File:Diag1angularmom.png]]

Now, the new position of the mass 1 is just

:<math> \vec{r_{mwrlr}} = <d/2(cos(\theta), d/2sin(\theta), 0)> </math>

For Mass 2, it's the same but with an angle that is 180 degrees less than theta.

Now we have to find the arrangement of the first cylinder.

:<math> \theta_{f} = \theta_{i} + \vec{w_{1}} \times \Delta t </math>

:<math> \vec{r_{cyl}} = <b(sin(\theta)), b(cos(theta)), 0> </math>

Then the positions of the two masses are just these two vectors added together.

:<math> \vec{r_{m}} = \vec{r_{cyl}} + \vec{r_{mwrlr}} </math>

The link to the code: https://www.glowscript.org/#/user/danielisme18/folder/MyPrograms/program/angularMomentump1

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-04T01:59:12Z

DanOConnor: /* Computational Model for this problem */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

===Computational Model for this problem===
[[File:AngularMomentumGif.gif]]

Here the angular momentum points in the negative z-hat direction because the masses are moving clockwise (both Ltrans and Lrot)

In order to update the positions of the masses in this computational model, you need to find the new position of the masses with respect to the center that it is rotating around (in this case it is the axis which we used to calculate lrot) and you need the new position of the rod that is rotating.

To calculate the new position of the masses with respect to the axis they are rotating around (Lrot), we need to find the change in angle between the last iteration and the new one, then we need to use trig.

To find the new angle we can take the old angle and add it to w * deltat

:<math> \theta_{f} = \theta_{i} + \vec{w_{2}}\times \Delta t </math>

[[File:Diag1angularmom.png]]

Now, the new position of the mass 1 is just

:<math> \vec{r} = <d/2(cos(\theta), d/2sin(\theta), 0)> </math>

For Mass 2, it's the same but with an angle that is 180 degrees less than theta.

Now we have to find the arrangement of the first cylinder.

:<math> \theta_{f} = \theta_{i} + \vec{w_{1}} \times \Delta t </math>

:<math> \vec{r} = <b(sin(\theta)), b(cos(theta)), 0> </math>

The link to the code: https://www.glowscript.org/#/user/danielisme18/folder/MyPrograms/program/angularMomentump1

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-04T01:58:35Z

DanOConnor: /* Computational Model for this problem */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

===Computational Model for this problem===
[[File:AngularMomentumGif.gif]]

Here the angular momentum points in the negative z-hat direction because the masses are moving clockwise (both Ltrans and Lrot)

In order to update the positions of the masses in this computational model, you need to find the new position of the masses with respect to the center that it is rotating around (in this case it is the axis which we used to calculate lrot) and you need the new position of the rod that is rotating.

To calculate the new position of the masses with respect to the axis they are rotating around (Lrot), we need to find the change in angle between the last iteration and the new one, then we need to use trig.

To find the new angle we can take the old angle and add it to w * deltat

:<math> \theta_{f} = \theta_{i} + \vec{w_{2}}\times \Delta t </math>

[[File:Diag1angularmom.png]]

Now, the new position of the mass 1 is just

:<math> \vec{r} = <d/2(cos(\theta), d/2sin(\theta), 0)> </math>

For Mass 2, it's the same but with an angle that is 180 degrees less than theta.

Now we have to find the arrangement of the first cylinder.

:<math> \theta_{f} = \theta_{i} + vec{w_{1}} \times \Delta t </math>

:<math> \vec{r} = <b(sin(\theta)), b(cos(theta)), 0> </math>

The link to the code: https://www.glowscript.org/#/user/danielisme18/folder/MyPrograms/program/angularMomentump1

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-04T01:57:53Z

DanOConnor: /* Computational Model for this problem */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

===Computational Model for this problem===
[[File:AngularMomentumGif.gif]]

Here the angular momentum points in the negative z-hat direction because the masses are moving clockwise (both Ltrans and Lrot)

In order to update the positions of the masses in this computational model, you need to find the new position of the masses with respect to the center that it is rotating around (in this case it is the axis which we used to calculate lrot) and you need the new position of the rod that is rotating.

To calculate the new position of the masses with respect to the axis they are rotating around (Lrot), we need to find the change in angle between the last iteration and the new one, then we need to use trig.

To find the new angle we can take the old angle and add it to w * deltat

:<math> \theta_{f} = \theta_{i} + \vec{w_{2}}\times \Delta t </math>

[[File:Diag1angularmom.png]]

Now, the new position of the mass 1 is just

:<math> \vec{r} = <d/2(cos(\theta), d/2sin(\theta), 0)> </math>

For Mass 2, it's the same but with an angle that is 180 degrees less than theta.

Now we have to find the arrangement of the first cylinder.

:<math> \theta_{f} = \theta_{i} + vec{w_{1}} \times \Delta t </math>

:<math> \vec{r} = <L(sin(\theta)), L(cos(theta)), 0> </math>

The link to the code: https://www.glowscript.org/#/user/danielisme18/folder/MyPrograms/program/angularMomentump1

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-04T01:53:44Z

DanOConnor: /* Computational Model for this problem */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

===Computational Model for this problem===
[[File:AngularMomentumGif.gif]]

Here the angular momentum points in the negative z-hat direction because the masses are moving clockwise (both Ltrans and Lrot)

In order to update the positions of the masses in this computational model, you need to find the new position of the masses with respect to the center that it is rotating around (in this case it is the axis which we used to calculate lrot) and you need the new position of the rod that is rotating.

To calculate the new position of the masses with respect to the axis they are rotating around (Lrot), we need to find the change in angle between the last iteration and the new one, then we need to use trig.

To find the new angle we can take the old angle and add it to w * deltat

:<math> \theta_{f} = \theta_{i} + \vec{w}\times \Delta t </math>

[[File:Diag1angularmom.png]]

Now, the new position of the mass 1 is just

:<math> \vec{r} = <d/2(cos(\theta), d/2sin(\theta), 0)> </math>

For Mass 2, it's the same but with an angle that is 180 degrees less than \theta.

The link to the code: https://www.glowscript.org/#/user/danielisme18/folder/MyPrograms/program/angularMomentump1

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-04T01:52:35Z

DanOConnor: /* Computational Model for this problem */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

===Computational Model for this problem===
[[File:AngularMomentumGif.gif]]

Here the angular momentum points in the negative z-hat direction because the masses are moving clockwise (both Ltrans and Lrot)

In order to update the positions of the masses in this computational model, you need to find the new position of the masses with respect to the center that it is rotating around (in this case it is the axis which we used to calculate lrot) and you need the new position of the rod that is rotating.

To calculate the new position of the masses with respect to the axis they are rotating around (Lrot), we need to find the change in angle between the last iteration and the new one, then we need to use trig.

To find the new angle we can take the old angle and add it to w * deltat

:<math> \theta_{f} = \theta_{i} + \vec{w}\times \Delta t </math>

[[File:Diag1angularmom.png]]

Now, the new position of the mass 1 is just

:<math> \vec{r} = <d/2(cos(\theta), d/2sin(\theta), 0)> </math>

The link to the code: https://www.glowscript.org/#/user/danielisme18/folder/MyPrograms/program/angularMomentump1

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-04T01:50:18Z

DanOConnor: /* Computational Model for this problem */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

===Computational Model for this problem===
[[File:AngularMomentumGif.gif]]

Here the angular momentum points in the negative z-hat direction because the masses are moving clockwise (both Ltrans and Lrot)

In order to update the positions of the masses in this computational model, you need to find the new position of the masses with respect to the center that it is rotating around (in this case it is the axis which we used to calculate lrot) and you need the new position of the rod that is rotating.

To calculate the new position of the masses with respect to the axis they are rotating around (Lrot), we need to find the change in angle between the last iteration and the new one, then we need to use trig.

To find the new angle we can take the old angle and add it to w * deltat

:<math> \theta_{f} = \theta_{i} + \vec{w}\times \Delta t </math>

[[File:Diag1angularmom.png]]

The link to the code: https://www.glowscript.org/#/user/danielisme18/folder/MyPrograms/program/angularMomentump1

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

File:Diag1angularmom.png

2023-12-04T01:48:53Z

DanOConnor: This is for the problem on the total angular momentum page

== Summary ==
This is for the problem on the total angular momentum page

File:Diagram1.png

2023-12-04T01:48:04Z

DanOConnor: DanOConnor uploaded a new version of File:Diagram1.png

This picture shows a ball attached to a spring and the forces acting on the ball. A blue arrow (Fspring) points upwards while the white arrow (Fgrav) points down, towards the Earth. The net force would be Fspring - Fgrav, which would equal 0 in this case, since the ball is at rest. This means Fspring and Fgrav are equal.

Total Angular Momentum

2023-12-04T01:47:04Z

DanOConnor: /* Computational Model for this problem */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

===Computational Model for this problem===
[[File:AngularMomentumGif.gif]]

Here the angular momentum points in the negative z-hat direction because the masses are moving clockwise (both Ltrans and Lrot)

In order to update the positions of the masses in this computational model, you need to find the new position of the masses with respect to the center that it is rotating around (in this case it is the axis which we used to calculate lrot) and you need the new position of the rod that is rotating.

To calculate the new position of the masses with respect to the axis they are rotating around (Lrot), we need to find the change in angle between the last iteration and the new one, then we need to use trig.

To find the new angle we can take the old angle and add it to w * deltat

:<math> \theta_{f} = \theta_{i} + \vec{w}\times \Delta t </math>

The link to the code: https://www.glowscript.org/#/user/danielisme18/folder/MyPrograms/program/angularMomentump1

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-04T01:46:22Z

DanOConnor: /* Computational Model for this problem */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

===Computational Model for this problem===
[[File:AngularMomentumGif.gif]]

Here the angular momentum points in the negative z-hat direction because the masses are moving clockwise (both Ltrans and Lrot)

In order to update the positions of the masses in this computational model, you need to find the new position of the masses with respect to the center that it is rotating around (in this case it is the axis which we used to calculate lrot) and you need the new position of the rod that is rotating.

To calculate the new position of the masses with respect to the axis they are rotating around (Lrot), we need to find the change in angle between the last iteration and the new one, then we need to use trig.

To find the new angle we can take the old angle and add it to w * deltat

:<math> \theta = \theta + \vec{w}\times \Delta t </math>

The link to the code: https://www.glowscript.org/#/user/danielisme18/folder/MyPrograms/program/angularMomentump1

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-04T01:46:00Z

DanOConnor: /* Computational Model for this problem */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

===Computational Model for this problem===
[[File:AngularMomentumGif.gif]]

Here the angular momentum points in the negative z-hat direction because the masses are moving clockwise (both Ltrans and Lrot)

In order to update the positions of the masses in this computational model, you need to find the new position of the masses with respect to the center that it is rotating around (in this case it is the axis which we used to calculate lrot) and you need the new position of the rod that is rotating.

To calculate the new position of the masses with respect to the axis they are rotating around (Lrot), we need to find the change in angle between the last iteration and the new one, then we need to use trig.

To find the new angle we can take the old angle and add it to w * deltat

:<math> \theta = \vec{w}\times \Delta t </math>

The link to the code: https://www.glowscript.org/#/user/danielisme18/folder/MyPrograms/program/angularMomentump1

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-04T01:45:41Z

DanOConnor: /* Computational Model for this problem */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

===Computational Model for this problem===
[[File:AngularMomentumGif.gif]]

Here the angular momentum points in the negative z-hat direction because the masses are moving clockwise (both Ltrans and Lrot)

In order to update the positions of the masses in this computational model, you need to find the new position of the masses with respect to the center that it is rotating around (in this case it is the axis which we used to calculate lrot) and you need the new position of the rod that is rotating.

To calculate the new position of the masses with respect to the axis they are rotating around (Lrot), we need to find the change in angle between the last iteration and the new one, then we need to use trig.

To find the new angle we can take the old angle and add it to w * deltat

:<math> \theta = \vec{w}\times \delta t </math>

The link to the code: https://www.glowscript.org/#/user/danielisme18/folder/MyPrograms/program/angularMomentump1

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-04T01:45:26Z

DanOConnor: /* Computational Model for this problem */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

===Computational Model for this problem===
[[File:AngularMomentumGif.gif]]

Here the angular momentum points in the negative z-hat direction because the masses are moving clockwise (both Ltrans and Lrot)

In order to update the positions of the masses in this computational model, you need to find the new position of the masses with respect to the center that it is rotating around (in this case it is the axis which we used to calculate lrot) and you need the new position of the rod that is rotating.

To calculate the new position of the masses with respect to the axis they are rotating around (Lrot), we need to find the change in angle between the last iteration and the new one, then we need to use trig.

To find the new angle we can take the old angle and add it to w * deltat

:<math> \theta = \vec{w}\times deltat </math>

The link to the code: https://www.glowscript.org/#/user/danielisme18/folder/MyPrograms/program/angularMomentump1

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-04T01:45:06Z

DanOConnor: /* Computational Model for this problem */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

===Computational Model for this problem===
[[File:AngularMomentumGif.gif]]

Here the angular momentum points in the negative z-hat direction because the masses are moving clockwise (both Ltrans and Lrot)

In order to update the positions of the masses in this computational model, you need to find the new position of the masses with respect to the center that it is rotating around (in this case it is the axis which we used to calculate lrot) and you need the new position of the rod that is rotating.

To calculate the new position of the masses with respect to the axis they are rotating around (Lrot), we need to find the change in angle between the last iteration and the new one, then we need to use trig.

To find the new angle we can take the old angle and add it to w * deltat

:<math> \theta = \vec{w}\times delta t </math>

The link to the code: https://www.glowscript.org/#/user/danielisme18/folder/MyPrograms/program/angularMomentump1

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-04T01:44:53Z

DanOConnor: /* Computational Model for this problem */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

===Computational Model for this problem===
[[File:AngularMomentumGif.gif]]

Here the angular momentum points in the negative z-hat direction because the masses are moving clockwise (both Ltrans and Lrot)

In order to update the positions of the masses in this computational model, you need to find the new position of the masses with respect to the center that it is rotating around (in this case it is the axis which we used to calculate lrot) and you need the new position of the rod that is rotating.

To calculate the new position of the masses with respect to the axis they are rotating around (Lrot), we need to find the change in angle between the last iteration and the new one, then we need to use trig.

To find the new angle we can take the old angle and add it to w * deltat

:<math> \theta = \vec{w}\times t </math>

The link to the code: https://www.glowscript.org/#/user/danielisme18/folder/MyPrograms/program/angularMomentump1

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-04T01:44:30Z

DanOConnor: /* Computational Model for this problem */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

===Computational Model for this problem===
[[File:AngularMomentumGif.gif]]

Here the angular momentum points in the negative z-hat direction because the masses are moving clockwise (both Ltrans and Lrot)

In order to update the positions of the masses in this computational model, you need to find the new position of the masses with respect to the center that it is rotating around (in this case it is the axis which we used to calculate lrot) and you need the new position of the rod that is rotating.

To calculate the new position of the masses with respect to the axis they are rotating around (Lrot), we need to find the change in angle between the last iteration and the new one, then we need to use trig.

To find the new angle we can take the old angle and add it to w * deltat

:<math> \vec{r} = \vec{w}\times t </math>

The link to the code: https://www.glowscript.org/#/user/danielisme18/folder/MyPrograms/program/angularMomentump1

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-04T01:43:43Z

DanOConnor: /* Computational Model for this problem */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

===Computational Model for this problem===
[[File:AngularMomentumGif.gif]]

Here the angular momentum points in the negative z-hat direction because the masses are moving clockwise (both Ltrans and Lrot)

In order to update the positions of the masses in this computational model, you need to find the new position of the masses with respect to the center that it is rotating around (in this case it is the axis which we used to calculate lrot) and you need the new position of the rod that is rotating.

To calculate the new position of the masses with respect to the axis they are rotating around (Lrot), we need to find the change in angle between the last iteration and the new one, then we need to use trig.

To find the new angle we can take the old angle and add it to w * deltat

:<math> \vec{r} = \vec{w}\times\t </math>

The link to the code: https://www.glowscript.org/#/user/danielisme18/folder/MyPrograms/program/angularMomentump1

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-04T01:41:34Z

DanOConnor: /* Computational Model for this problem */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

===Computational Model for this problem===
[[File:AngularMomentumGif.gif]]

Here the angular momentum points in the negative z-hat direction because the masses are moving clockwise (both Ltrans and Lrot)

In order to update the positions of the masses in this computational model, you need to find the new position of the masses with respect to the center that it is rotating around (in this case it is the axis which we used to calculate lrot) and you need the new position of the rod that is rotating.

To calculate the new position of the masses with respect to the axis they are rotating around (Lrot), we need to find the change in angle between the last iteration and the new one, then we need to use trig.

To find the new angle we can take the old angle and add it to w * deltat

<math> <math/>

The link to the code: https://www.glowscript.org/#/user/danielisme18/folder/MyPrograms/program/angularMomentump1

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-04T01:34:08Z

DanOConnor: /* Computational Model for this problem */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

===Computational Model for this problem===
[[File:AngularMomentumGif.gif]]

Here the angular momentum points in the negative z-hat direction because the masses are moving clockwise (both Ltrans and Lrot)

In order to update the positions of the masses in this computational model, you need to find the new position of the masses with respect to the center that it is rotating around (in this case it is the axis which we used to calculate lrot) and you need the new position of the rod that is rotating. These can be calculated with simple trig and the change in degrees given by deltat * w.

The link to the code: https://www.glowscript.org/#/user/danielisme18/folder/MyPrograms/program/angularMomentump1

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-04T01:18:00Z

DanOConnor: /* Computational Model for this problem */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

===Computational Model for this problem===
[[File:AngularMomentumGif.gif]]

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

File:AngularMomentumGif.gif

2023-12-04T01:17:20Z

DanOConnor: This illustrates the above problem. The code is linked below

== Summary ==
This illustrates the above problem. The code is linked below

File:Giphy.gif

2023-12-04T01:12:34Z

DanOConnor:

Total Angular Momentum

2023-12-04T01:12:02Z

DanOConnor: /* Difficult */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

===Computational Model for this problem===

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-03T23:38:26Z

DanOConnor:

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===We can't have angular momentum without an axis===
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-03T23:37:43Z

DanOConnor: /* The Main Idea */

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convenient to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

== We can't have angular momentum without an axis ==
Just like picking a coordinate system for a Free Body Diagram it is important to pick a point where the system rotates. You can pick any point in space; however, it may not really help you much with determining what's actually going to happen in a given situation. If you wanted to be able to predict motion and the effect of torque on motion it is best to pick a point that the system actually will rotate around. Your choice should be relatively simple.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-03T23:27:19Z

DanOConnor:

Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convienent to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]

Total Angular Momentum

2023-12-03T19:41:47Z

DanOConnor:

Claimed by Daniel O'Connor Fall 2023

==The Main Idea==

[[File:Translational and Rotational Angular Momentum.png]]

In the same way it can be convienent to analyze the linear motion of a system via the changes in the linear momentum of the system, it can be useful to use the concept of angular momentum to describe the motion of rotating systems. In general, momentum is a useful concept because it is usually possible to find a system in which the total momentum of the system is conserved - that is, no external force is acting on the system. However, even when momentum isn't conserved, it still provides a useful relationship between the rate of change of an object's motion and the force applied to the object. Angular momentum is useful for this same reason and can be utilized in a similar way.

===A Mathematical Model===

'''Single Particle Systems'''

For a single particle revolving about a center of rotation, the angular momentum of the particle is expressed in terms of the particle's translational momentum about the center, as shown below:

:<math> \vec{L} = \vec{r}\times\vec{p} </math>

'''Multiparticle Systems'''

The same technique can also be used to describe the total angular momentum of a multi particle system revolving about a center of rotation. In this case, the total angular momentum is simply the sum of the angular momentum for each particle:

:<math> \vec{L_{tot}} = \sum_{j=1}^n \vec{r_j}\times\vec{p_j} </math>

'''Continuous Masses'''

If you imagine letting the summation for the multiparticle system approach infinity, that is if you were to fill some finite volume with an infinite number of infinitesimally small particles, you would create a continuous distribution of mass rotating about the same central axis. This is how we model the angular momentum of extended objects, or objects that cannot be represented by points. When this is done, you arrive at the following equation:

<math> \vec{L} = I\vec{\omega} </math>

Here <math> I </math> is the rotational inertia of the object (For more info see Rotational Inertia) and <math> \omega </math> is the angular frequency.

It is also Important to note that an object could be treated as a point particle about one axis and an extended object about another, i.e. the Earth rotating while revolving around the sun. In this case, it is useful to separate the object's angular momentum into translational and "spin" components (for more info see Translational & Spin Angular Momentum)

===A Computational Model===

You can visualize this topic of total angular momentum with this code of the total angular momentum of a binary star. You can see the rotational angular momentum along with the translational angular momentum.

[[File:Screen_Shot_2015-12-02_at_1.36.42_AM.png]]

This screenshot shows the code in action but you can check it out with this link: '''https://trinket.io/glowscript/49129c12fd'''

==Examples==

These examples will help to solidify the difference between the different components of total angular momentum.

===Simple===

A ball falls straight down in the xy plane. Its momentum is shown by the red arrow. What is the direction of the ball's total angular momentum about location A?

[[File:Simple final.png]]

When attempting to solve this question, it is important to recognize that there is no rotational angular momentum, because there is no rotation about the center of mass. The only thing that is happening is that the center of mass is translating from some point A. In this case since there is only translational angular momentum, we would simply find the direction of the total angular momentum by using our right hand rule [hint: r points from A to the ball, and the momentum is pointing in the -y direction]

The direction of the ball's total angular momentum is in the -z direction.

===Middling===

This example shows the importance of understanding the difference between rotational and translational angular momentum.

[[File:Easy.png]]

[[File:simple example.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Screen Shot 2015-11-25 at 3.19.38 PM.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Simple example 1.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
'''

Due to the fact that...

[[File:Total Angular Momentum.png]]

We calculated that our Lrot is zero, our total angular momentum is just based on translational angular momentum. So in this case, total angular momentum = translational angular momentum. So total angular momentum is 9.72 kgm^2/s, with the same direction, into the page.

===Difficult===

This problem shows an example of total angular momentum being based off both translational angular momentum and rotational angular momentum.

[[File:Middle example 1.png]]

[[File:Middle example 2.png]]

'''a) Calculate Lrot (both magnitude and direction)
'''

[[File:Middle rotational.png]]

'''b) Calculate Ltrans,B (both magnitude and direction)
'''

[[File:Middle translational.png]]

'''c) Calculate Ltotal,B (both magnitude and direction)
''

The total angular momentum is rotational + translational so it is <0,0,-11.16> kgm^2/s

==Connectedness==

This topic is connected to my major (biomedical engineering)), because it is important to understand the basics before attempting to solve the bigger picture. In terms of angular momentum, it is important to understand the breakdown of translational and rotational before attempting to solve complex problems involving conservation of angular momentum and more. It can be seen in so many examples, from the rotation of a figure skater to a a yoyo.

Total angular momentum is very interesting to witness in the orbit of planets and satellites.
[[File:Application of Total Angular Momentum.png]]

This image shows the translational angular momentum of the Earth (relative to the location of the Sun) and the rotational angular momentum (relative to the center of mass of the Earth).

It is also important to note that for point particle systems that there is no rotational angular momentum, and only translational angular momentum. This is important, because the total angular momentum for a point particle system is just simply translational angular momentum.

Understanding the topic of total angular momentum is extremely important in applying the conservation of angular momentum. Due to the fact that angular momentum is conserved, then it is important to note that if there is net force on some body directed towards a fix point, the center, then there is no torque on the body with respect to the center, and the angular momentum of the body about the center is constant. There is a very useful application of constant angular momentum, specifically seen in dealing with the orbits of planets and satellites. This concept is also used for the Bohr model of the atom.

==History==

Newton, in the Principia, hinted at angular momentum in his examples of the First Law of Motion,

''"A top, whose parts by their cohesion are perpetually drawn aside from rectilinear motions, does not cease its rotation, otherwise than as it is retarded by the air. The greater bodies of the planets and comets, meeting with less resistance in more free spaces, preserve their motions both progressive and circular for a much longer time."
''
However, his geometric proof of the Law of Areas is an outstanding example of Newton's genius, and indirectly proves angular momentum conservation in the case of a central force.

In 1736 Euler, like Newton, touched on some of the equations of angular momentum in his Mechanica without further developing them.

Bernoulli wrote in a 1744 letter of a "moment of rotational motion", possibly the first conception of angular momentum as we now understand it.

In 1799, Pierre-Simon Laplace first realized that a fixed plane was associated with rotation — his invariable plane.

Louis Poinsot in 1803 began representing rotations as a line segment perpendicular to the rotation, and elaborated on the "conservation of moments".

In 1852 Léon Foucault used a gyroscope in an experiment to display the Earth's rotation.

William J. M. Rankine's 1858 Manual of Applied Mechanics defined angular momentum in the modern sense for the first time:

''"...a line whose length is proportional to the magnitude of the angular momentum, and whose direction is perpendicular to the plane of motion of the body and of the fixed point, and such, that when the motion of the body is viewed from the extremity of the line, the radius-vector of the body seems to have right-handed rotation."
''

== See also ==

===Further reading===

Books and other print media that cover this topic in more depth:

Elementary Theory of Angular Momentum (Dover Books on Physics) by M.E. Rose

Matter and Interactions by Ruth W. Chabay and Bruce A. Sherwood

http://chaos.utexas.edu/wp-uploads/2012/03/Angular_Momentum_21.pdf

===Video Content===

Videos on Total Angular Momentum:

https://www.youtube.com/watch?v=8SfRmqSQENU&index=34&list=PL9HgJKLOnKxedh-yIp7FDzUTwZeTeoR-Y

https://www.youtube.com/watch?v=nFSMu3bxXVA

https://www.youtube.com/watch?v=diZDoY07LG4

https://www.youtube.com/watch?v=iWSu6U0Ujs8

===External links===

These are some internet articles that can show more animations and pictures to help understand this concept

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

==References==

https://www.chegg.com/homework-help

http://www.sparknotes.com/physics/rotationalmotion/angularmomentum/section1.rhtml

http://www.phy.duke.edu/~lee/P53/sys.pdf

http://farside.ph.utexas.edu/teaching/301/lectures/node120.html

https://www.physics.purdue.edu/webapps/index.php/course_document/index/phys172/1332/135/9703

http://hyperphysics.phy-astr.gsu.edu/hbase/amom.html

http://www.sparknotes.com/testprep/books/sat2/physics/chapter10section6.rhtml

Professor Gumbart [Georgia Institute of Technology] Lecture Notes

Matter and Interactions 4th edition. Full Citation: Chabay, Ruth W., and Bruce A. Sherwood. Matter and Interactions. Hoboken, NJ: Wiley, 2011. Print.

https://en.wikipedia.org/wiki/Angular_momentum

[[Category:Which Category did you place this in?]]