Why does photons of a given frequency satisfy the Boltzmann distribution?

In summary: In the classical limit, the two distributions become indistinguishable.In summary, the interpretation of a mode of frequency ##\nu## having energy ##E_n = h \nu## as corresponding to ##n## photons of energy ##h \nu## leads to a probability distribution of ##p(n) = e^{-nh\nu}/Z##, which follows Boltzmann statistics. However, in the classical limit, this distribution becomes similar to the Bose-Einstein distribution, which is the correct approach for dealing with photons as bosons. The confusion may arise from the difference between considering modes vs individual photons and the summation over all n in the Bose-Einstein distribution.
  • #1
center o bass
560
2
A mode of frequency ##\nu## has energy ##E_n = h \nu##. In terms of photons, the interpretation that I have read several places, is that this correspond to ##n## photons of energy ##h \nu##. Furthermore, it is stated that the probabilty of finding ##n## photons at frequency ##\nu## is given by
$$p(n) = e^{-nh\nu}/Z,$$
where Z is the partition function (for example in: http://disciplinas.stoa.usp.br/pluginfile.php/48089/course/section/16461/qsp_chapter10-plank.pdf)

This correspond to Boltzmann statistics, and I'm a bit confused by this since photons are supposedly bosons. Should'nt this instead be Bose-Einstein statistics?
 
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  • #2
Yes, Bose-Einstein statistics are the correct approach. However, in the classical limit the differences between the two distributions vanish. For example for bosonic atoms, there is not really a difference between the distributions for high temperatures and diluted gases.

For photons, using Boltzmann statistics is fine if you are dealing with large energies because the additional "-1" becomes negligible and Maxwell-Boltzmann statistics become a good approximation to Bose-Einstein statistics.
 
  • #3
Cthugha said:
Yes, Bose-Einstein statistics are the correct approach. However, in the classical limit the differences between the two distributions vanish. For example for bosonic atoms, there is not really a difference between the distributions for high temperatures and diluted gases.

For photons, using Boltzmann statistics is fine if you are dealing with large energies because the additional "-1" becomes negligible and Maxwell-Boltzmann statistics become a good approximation to Bose-Einstein statistics.

I agree that this is correct in the classical limit. However in http://disciplinas.stoa.usp.br/pluginfile.php/48089/course/section/16461/qsp_chapter10-plank.pdf the complete Planck law is derived by assuming that the probability that a single mode is in a state of energy E=nhν (a state of n photons) is given by a Boltzmann distribution. Hence, the derivation does not consider any limit.
 
  • #4
Sorry, I do not have access to that PDF file on my phone right now, but are you completely sure that the partition function Z they use is really the classical Maxwell-Boltzmann one?

If they just consider the number of photons in each energy state, they apply BE statistics. If they also take multiplicities into account and you see a lot of factorials, it is most likely the classical partition function.
 
  • #5
Cthugha said:
Sorry, I do not have access to that PDF file on my phone right now, but are you completely sure that the partition function Z they use is really the classical Maxwell-Boltzmann one?

If they just consider the number of photons in each energy state, they apply BE statistics. If they also take multiplicities into account and you see a lot of factorials, it is most likely the classical partition function.

Might the confusion lie in the difference between modes vs photons or photons at frequency ##\nu## vs photons at any frequency?

To quote directly what is stated:

"The probability that a single mode has energy ##E_n = n h\nu## is given by
$$p(n) = \frac{e^{-E_n/kT}}{\sum_{n=0}^\infty e^{-E_n/kT}}$$
where the denominator ensures that the sum of probabilities is unity, the standard normalization procedure. In the language of photons this is the probability that the state contains ##n## photons of frequency ##\nu##. "
 
  • #6
center o bass said:
A mode of frequency ##\nu## has energy ##E_n = h \nu##. In terms of photons, the interpretation that I have read several places, is that this correspond to ##n## photons of energy ##h \nu##. Furthermore, it is stated that the probabilty of finding ##n## photons at frequency ##\nu## is given by
$$p(n) = e^{-nh\nu}/Z,$$
where Z is the partition function (for example in: http://disciplinas.stoa.usp.br/pluginfile.php/48089/course/section/16461/qsp_chapter10-plank.pdf)

This correspond to Boltzmann statistics, and I'm a bit confused by this since photons are supposedly bosons. Should'nt this instead be Bose-Einstein statistics?
Bose-Einstein distribution involves an average over all n, giving the probability of a given frequency. It is the summation over all n that gives the characteristic Bose-Einstein form of the distribution.

When n is fixed, there is no any difference between classical (Maxwell-Boltzmann) and quantum (Bose-Einstein) statistics.
 

FAQ: Why does photons of a given frequency satisfy the Boltzmann distribution?

1. What is the Boltzmann distribution and how does it relate to photons?

The Boltzmann distribution is a statistical probability distribution that describes the distribution of particles in a system at thermal equilibrium. It is often used to describe the distribution of energy levels in a system, including the energy levels of photons. This means that photons of a given frequency will follow the Boltzmann distribution, which determines the likelihood of finding them at different energy levels.

2. Why is it important for photons to satisfy the Boltzmann distribution?

The Boltzmann distribution is important because it describes the behavior of particles in a thermodynamic system, including photons. By following this distribution, photons are able to achieve thermal equilibrium with their surroundings, which is crucial for understanding and predicting the behavior of light in various systems.

3. How does the Boltzmann distribution affect the emission and absorption of photons?

The Boltzmann distribution directly affects the emission and absorption of photons. It determines the relative probabilities of photons being emitted or absorbed at different energy levels, which ultimately determines the intensity and spectral distribution of light emitted or absorbed by a system.

4. What factors influence the Boltzmann distribution of photons?

The Boltzmann distribution of photons is influenced by several factors, including temperature, energy levels of the system, and the number of particles present. As these factors change, the distribution of photons will also change, resulting in different intensities and spectral distributions of light.

5. Can the Boltzmann distribution be applied to other types of particles besides photons?

Yes, the Boltzmann distribution can be applied to any type of particle in a thermodynamic system, such as atoms, molecules, or even subatomic particles. It describes the distribution of energy levels and probabilities of finding particles at different energy states, and is a fundamental concept in statistical mechanics and thermodynamics.

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