Non equilibrium boson distribution function

In summary, the boson distribution function in statistical mechanics takes the form ##f = \frac{1}{e^{E/T} - 1}## in the case of zero chemical potential. When considering the non-equilibrium variant, this form is generalized to ##f = \frac{1}{e^{\frac{E}{T(1+ \Theta)}} - 1}##, where ##\Theta## is some function. This form is likely an approximation for small deviations from local equilibrium, and can be derived from Onsager's reciprocal relations and the Bose-Einstein partition statistics.
  • #1
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In statistical mechanics the boson distribution function has the well known form
##f = \frac{1}{e^{E/T} - 1},##
(in the special case of zero chemical potential). As one considers the non-equilibrium variant this generalize to
##f = \frac{1}{e^{\frac{E}{T(1+ \Theta)}} - 1},##
for some function ##\Theta##. Now, is there any intuitive (or rigorous) explanation of why this is the correct form for the non-equilibrium distribution?
 
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  • #2
Given that I haven't studied NE thermodynamics, this is my attempt:

If the expression is correct (and I haven't found a reference), it is likely correct as an approximation for small deviations from a local equilibrium. Then we can apply Onsager's relations. Onsager looked at the the entropy density s, so

du = T ds

when neglecting chemical potential. [ http://en.wikipedia.org/wiki/Onsager_reciprocal_relations ]

The classical derivation of the Bose-Einstein partition statistics uses S = k lnW to identify β = 1/kT from dE = T dS (again neglecting C.P.). [ http://en.wikipedia.org/wiki/Maxwell–Boltzmann_statistics#Derivation_from_canonical_ensemble ] You have normalized k =1.

Small perturbations in entropy density would show up as perturbations in the energy density du = T (1 + Θ) ds under the approximation.* We get E/T(1+Θ) where it was previously E/T.

* The convenient functional form, since T = constant is a possible constraint.
 
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Related to Non equilibrium boson distribution function

1. What is a non-equilibrium boson distribution function?

A non-equilibrium boson distribution function is a mathematical function that describes the distribution of bosonic particles in a system that is not in thermodynamic equilibrium. It takes into account factors such as external forces, non-conservative interactions, and changes in temperature or density over time.

2. How is a non-equilibrium boson distribution function different from an equilibrium one?

An equilibrium boson distribution function assumes that the system is in a steady state, with no external forces or changes in temperature or density over time. A non-equilibrium distribution function takes into account these factors, which can significantly affect the distribution of bosons in the system.

3. What are the applications of non-equilibrium boson distribution functions?

Non-equilibrium boson distribution functions are commonly used in the field of condensed matter physics to describe the behavior of bosonic particles in systems such as superfluids, superconductors, and Bose-Einstein condensates. They are also used in quantum field theory and high-energy physics to study the behavior of particles in non-equilibrium states.

4. How is a non-equilibrium boson distribution function calculated?

The calculation of a non-equilibrium boson distribution function involves solving a set of differential equations that describe the dynamics of the bosonic particles in the system. These equations take into account factors such as external forces, non-conservative interactions, and changes in temperature or density over time.

5. What are the challenges in studying non-equilibrium boson distribution functions?

One of the main challenges in studying non-equilibrium boson distribution functions is the complexity of the mathematical equations involved. Solving these equations can be computationally intensive and require advanced mathematical techniques. Additionally, experimental verification of theoretical predictions can be difficult due to the delicate nature of systems in non-equilibrium states.

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