What is the Average Energy per Photon at Thermal Equilibrium?

In summary, the average energy per photon for photons in thermal equilibrium with a cavity at temperature T is given by the equation E/V = (8π(kT)^3)/(15(hc)^3). To find the energy per photon, you must also find the number of photons per volume and divide. This results in the final equation, E/N = kT(π^4)/(15(2.41)). For part (b), you can simply plug in the value for T and calculate the average photon energy in electron volts.
  • #1
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Homework Statement


(a) Find the average energy per photon for photons in thermal equilibrium with a cavity at temperature T.
(b) Calculate the average photon energy in electron volts at T = 6000K.

Homework Equations


[tex] u(E)dE = \frac{8 \pi}{(hc)^3} \frac{E^3 dE}{e^{E/k_B T} - 1}[/tex]

The Attempt at a Solution



Integrate both sides of the equation.
[tex] \frac{E}{V} = \int_0^\infty u(E)dE = \int_0^\infty \frac{8 \pi}{(hc)^3} \frac{E^3 dE}{e^{E/k_B T} - 1}[/tex]

Use the fact that
[tex]\frac{z^3 dz}{e^z - 1} = \frac{\pi^4}{15}[/tex]

and that the equation can be rewritten as
[tex] \frac{8 \pi (k_{B}T)^3}{(hc)^3} \int_0^\infty \frac{ (\frac{E}{k_B T})^3 dE}{e^{E/k_B}-1} [/tex]

which finally gives
[tex] \frac{E}{V} = \frac{8 \pi (k_{B}T)^3}{(hc)^3} \frac{\pi^4}{15}[/tex]

Did I do this right?

Part b will be easy, just plug in the value for T if (a) is right.
 
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  • #2
Ok, your approach so far is good, but you've missed three factors of kT (check your units!). Now you're asked to find the energy per photon, and you've found the total energy per volume, so you must now find the number of photons per volume and divide.
 
  • #3
Whoops, must have missed translating the cubed into typing because it's on my paper.

Okay, so I should find N/V and divide. So for N/V
[tex]\frac{N}{V} = \int_0^\infty n(E)dE = \int_0^\infty g(E)f_BE(E)dE[/tex]
and after some algebra
[tex] \frac{N}{V} = \frac{8 \pi}{(hc)^3}(k_B)^2 \int_0^\infty \frac{z^2}{e^z - 1}[/tex]
where
[tex]z= \frac{E}{k_B T}[/tex]
and since
[tex]\int_0^\infty \frac{z^2}{e^z - 1} = 2.41[/tex]
the number per volume becomes
[tex]\frac{N}{V} = \frac{8 \pi}{(hc)^3}(k_B)^2 (2.41)[/tex]
after taking the energy per volume and dividing it by the number per volume
[tex] \frac{E}{N} = k_B T \frac{\pi^4}{15(2.41)}[/tex]
 
  • #4
Which is of course just what you would expect: kT times some number of order one. This is because the only energy scale in the problem is kT.
 
  • #5
THe average energy per photon is simply

[tex]\langle E\rangle =kT\frac{\zeta(4)\Gamma(4)}{\zeta(3)\Gamma(3)} [/tex]

Daniel.
 

What is Bose-Einstein Statistics?

Bose-Einstein Statistics is a type of statistical mechanics that describes the behavior of a large number of identical particles, such as atoms or subatomic particles, in a system. It was developed by Satyendra Nath Bose and Albert Einstein in the 1920s.

What is the main difference between Bose-Einstein Statistics and other statistical mechanics?

The main difference is that Bose-Einstein Statistics allows for multiple particles to occupy the same quantum state, while other statistical mechanics, such as Maxwell-Boltzmann Statistics, do not. This is known as the Bose-Einstein condensate and leads to unique behaviors at very low temperatures.

What types of particles follow Bose-Einstein Statistics?

Particles that follow Bose-Einstein Statistics are known as bosons. These include particles with integer spin, such as photons, gluons, and some atoms. Fermions, on the other hand, follow a different type of statistics called Fermi-Dirac Statistics.

What is the significance of Bose-Einstein Statistics in the study of quantum mechanics?

Bose-Einstein Statistics is an important tool in understanding the behavior of quantum systems, particularly at very low temperatures. It has been used to explain phenomena such as superfluidity and superconductivity, and has applications in fields such as condensed matter physics, cosmology, and quantum computing.

How is Bose-Einstein Statistics related to the Bose-Einstein distribution?

The Bose-Einstein distribution is a mathematical function that describes the probability of finding a particle in a certain energy state at a given temperature. It is derived from Bose-Einstein Statistics and is used to calculate various thermodynamic properties of a system, such as the average number of particles in a particular state.

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