The Energy Principle: Difference between revisions
No edit summary |
No edit summary |
||
Line 18: | Line 18: | ||
There are many ways to use the energy principle; most of the problems you will encounter will have no work acting on the system and no transfer of heat, thus E<sub>sys,initial</sub> = E<sub>sys,final</sub>. Otherwise you will use E<sub>sys,initial</sub> + Wsurr+Q = E<sub>sys,final</sub>. | There are many ways to use the energy principle; most of the problems you will encounter will have no work acting on the system and no transfer of heat, thus E<sub>sys,initial</sub> = E<sub>sys,final</sub>. Otherwise you will use E<sub>sys,initial</sub> + Wsurr+Q = E<sub>sys,final</sub>. | ||
The first step in using the Energy Principle is to identify which initial and final energies have values in the equation. You can eliminate the values that are not present in the equation for the specific problem in order to simplify the solution of the problem. Additionally there may be multiple potential energies in the scenario that need to be included when solving the equation including Spring Potential Energy, Gravitational Potential Energy, Electric Potential Energy, and Gravitational Potential Energy near the surface of the Earth. Generally, if an initial or final state has zero velocity, the kinetic energy will be zero for that state. It's also key to note that potential energy is zero at very large distances. | The first step in using the Energy Principle is to identify which initial and final energies have values in the equation. You can eliminate the values that are not present in the equation for the specific problem in order to simplify the solution of the problem. Additionally there may be multiple potential energies in the scenario that need to be included when solving the equation including Spring Potential Energy, Gravitational Potential Energy, Electric Potential Energy, and Gravitational Potential Energy near the surface of the Earth. Generally, if an initial or final state has zero velocity, the kinetic energy will be zero for that state. It's also key to note that potential energy is zero at very large distances. | ||
The basic equation involving only kinetic and potential energy will often look like the following equation: | |||
Esys=(K1+K2+K3+…)+(U1,2+U1,3+U2,3+…) | |||
The eqations involving more energies can be seen in the Mathematical Models section. | |||
[[File:hydrogen atom.jpg|middle]] [[File:asteroidEarth.png|middle]] | [[File:hydrogen atom.jpg|middle]] [[File:asteroidEarth.png|middle]] |
Revision as of 13:41, 17 April 2016
claimed by Sunil Mutyala
The basis of the energy principle can be described with the statement, "energy can neither be created nor destroyed."
The energy principle is used to describe changes in energy on a system. These energies can take numerous different forms including Kinetic Energy, Potential Energy, Chemical Energy, Rest Energy, and Thermal Energy.
The Main Idea
The Energy Principle, also referred to as The First Law of Thermodynamics, defines the transfer of energy between systems. It is defined with the fact that the change of the energy of system is equal to the work surrounding in addition to heat transfers from the surroundings as well. This principle is defined with the equation
ΔEsys=Wsurr+Q
There are many ways to use the energy principle; most of the problems you will encounter will have no work acting on the system and no transfer of heat, thus Esys,initial = Esys,final. Otherwise you will use Esys,initial + Wsurr+Q = Esys,final. The first step in using the Energy Principle is to identify which initial and final energies have values in the equation. You can eliminate the values that are not present in the equation for the specific problem in order to simplify the solution of the problem. Additionally there may be multiple potential energies in the scenario that need to be included when solving the equation including Spring Potential Energy, Gravitational Potential Energy, Electric Potential Energy, and Gravitational Potential Energy near the surface of the Earth. Generally, if an initial or final state has zero velocity, the kinetic energy will be zero for that state. It's also key to note that potential energy is zero at very large distances. The basic equation involving only kinetic and potential energy will often look like the following equation: Esys=(K1+K2+K3+…)+(U1,2+U1,3+U2,3+…) The eqations involving more energies can be seen in the Mathematical Models section.
Mathematical Models
NOTE: These are a lot of equations, but don't get overwhelmed. You simply have to pick and choose which ones are necessary for the problem given; examples are shown below. For in-depth explanations on each type of energy, look at the associated pages on the Main Page or click on the links in the 'See also' section below.
The Energy Principle
EQ 1: [math]\displaystyle{ {∆E} = {Q + W} }[/math] where [math]\displaystyle{ {Q} }[/math] is heat and [math]\displaystyle{ {W} }[/math] is the amount of work acting on the system.
EQ 2: [math]\displaystyle{ {∆E} = {∆K + ∆E_{Rest} + ∆U + ∆E_{Thermal}} }[/math] - the different types of energy that can be associated with a given particle in a system. Not all have to be present.
EQ 3: [math]\displaystyle{ E_{Rest}=mc^2 }[/math] - Rest Energy, where m is the mass and c is the speed of light.
EQ 4: [math]\displaystyle{ K=\frac{1}{2}mv² }[/math] - Kinetic Energy, where m is the mass and v is the velocity (for speeds less than the speed of light).
EQ 5: [math]\displaystyle{ ∆E_{Thermal} = mC∆T }[/math] - Thermal energy, were m is the mass, C is the specific heat of water (4.2 J/g/K), and T is temperature.
Potential Energy Equations:
A Computational Model
This is a good visualization of kinetic, potential, and total energy.
Examples
Simple
A 1.3 kg book is pushed off a ledge and falls 4.22 m to the ground. What is its kinetic energy the instant that it hits the ground?
Middling
A 45 kg box moves along with a speed of 3.2 m/s. Someone comes up from behind and pushes it for 2.7 m while exerting a force of 185 N. What is the final speed of the box?
Difficult
The radius of Mars (from the center to just above the atmosphere) is 3220 km, and its mass is 2 ✕ 10^32 kg. An object is launched straight up from just above the atmosphere of Mars. What initial speed is needed so that when the object is far from Mars its final speed is 1000 m/s?
Connectedness
The Energy Principle can be used for a variety of situations; the fact that it can tell us something about the work acting on a system with only knowing about what energies are present (and vice versa) is what makes this such a fundamental principle. The energy principle is also used to describe the conservation of energy, which is something I find pretty interesting. Energy doesn't just disappear, it's simply converted into a different form. This topic has a huge connection to my major, Biology, because chemical energy (obtained from food) is necessary for a healthy and active body.
History
The concept of energy and its connection to the amount of work performed goes way back to the age of steam engines; physicists and engineers came up with this notion to describe how mechanically and thermally efficient their machines were. In the 1850's, people like William Thomson and William Rankine began to come up with terms like 'kinetic energy' and 'potential energy.' After the 1920's, this study of science became to be known as thermodynamics, the science of energy transformations. This led to the laws of thermodynamics, one of which relates to the conservation of energy.
See also
Potential Energy
Rest Mass Energy
Kinetic Energy
Work
Thermal Energy
Gravitational Potential Energy
Conservation of Energy
Spring Potential Energy
Further reading
Matter and Interactions By Ruth W. Chabay, Bruce A. Sherwood - Chapter 6
External links
http://hyperphysics.phy-astr.gsu.edu/hbase/conser.html#coneng
http://hyperphysics.phy-astr.gsu.edu/hbase/enecon.html
References
http://p3server.pa.msu.edu/coursewiki/doku.php?id=183_notes:define_energy
http://www.texample.net/tikz/examples/earth-orbit/
https://en.wikipedia.org/wiki/Conservation_of_energy
https://en.wikipedia.org/wiki/History_of_energy