Quantum Properties of Light: Difference between revisions

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<b>Spring 2022</b>
<b>Spring 2022</b>


Planck Relation
In the latter part of the 19th century, the classical description of light that had prevailed since the 17th century, began to fail in its explanatory power for the ever more precise measurements and phenomena being performed and observed in laboratories. The prime example of such failure is the so - called <b>Ultraviolet Catastrophe</b>. This term was first used by Paul Ehrenfest to refer to Rayleigh - Jeans law ability to predict experimental results below energies of 10^5 and its sudden unexplained divergence at energies close to the ultraviolet range in the electromagnetic spectrum.
 
Short Description of Topic
The Planck Relation helps us to be able to figure out the energy of a photon based on its frequency of radiation.


==The Main Idea==
==The Main Idea==

Revision as of 15:06, 23 April 2022

Giovanny Espitia, Spring 2022

In the latter part of the 19th century, the classical description of light that had prevailed since the 17th century, began to fail in its explanatory power for the ever more precise measurements and phenomena being performed and observed in laboratories. The prime example of such failure is the so - called Ultraviolet Catastrophe. This term was first used by Paul Ehrenfest to refer to Rayleigh - Jeans law ability to predict experimental results below energies of 10^5 and its sudden unexplained divergence at energies close to the ultraviolet range in the electromagnetic spectrum.

The Main Idea

The energy of a photon is related to the frequency of its radiation by Planck's constant, h. This has a value of 6.626*10^-34 Joules*seconds. Planck's relation allows us to find the energy of a photon, or its frequency (and wavelength) of its radiation.

A Mathematical Model

E=hv -h=6.626*10^-34 Joules*seconds

-E is the energy of a photon in Joules

-v is the frequency of the radiation of the proton in Hz

A Computational Model

Hyper physics has a program that allows users to input wavelength, frequency, or energy and find out the other two values. http://hyperphysics.phy-astr.gsu.edu/hbase/mod2.html#c3

Examples

Be sure to show all steps in your solution and include diagrams whenever possible

Simple

If a proton starts at frequency v, and its frequency increases, does its energy increase or decrease?

Its energy increases because E and v have a positive linear correlation. E=hv ?=h2v 2E=h2v

Middling

What is the energy of a single photon of orange light?

Orange light has a radiation frequency of 435 THz.

E=hv

E=( 435*10^12)(6.626*10^-34)

E=2.88*10^-18 Joules

Difficult

Connectedness

This relation allows us to understand the photoelectric effect (why some metals emit electrons when light is shined on them) and Planck's Law of Black Body Radiation.

Every day in the biomedical device industry, new forms of treatment for cancer are being used. Proton emission therapy is a current method. If photons were ever used to combat disease, Planck's Relation could help engineers to calculate their energy or radiation frequency and wavelength in order to adjust these values to get the ones desired.

History

Max Planck, a German Scientist discovered Planck's Relation. He published his paper in 1900. He was doing research and realized that matter could only emit or absorb radiation at certain discrete energy levels. He found a constant that described the distance between the energy levels.

Put this idea in historical context. Give the reader the Who, What, When, Where, and Why.

See also

Are there related topics or categories in this wiki resource for the curious reader to explore? How does this topic fit into that context?

Further reading

HyperPhysics page on Photoelectric Effect: http://hyperphysics.phy-astr.gsu.edu/hbase/mod2.html#c3

External links

A thorough example of a problem calculating the energy in a mole of photons using Planck's Relation: [1]

References

http://hyperphysics.phy-astr.gsu.edu/hbase/mod2.html#c3 https://www.youtube.com/watch?v=dSUvyERhtO8 This section contains the the references you used while writing this page