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Comparison of Three Types of Statistical Distributions

1. Introduction

In statistical mechanics, particles in thermal equilibrium follow different distribution laws depending on their nature.

The three important statistical distributions are:

2. Maxwell–Boltzmann Distribution

Applicable to classical distinguishable particles.

\[ f_{MB}(\epsilon) = e^{-\beta(\epsilon - \mu)} \]

3. Fermi–Dirac Distribution

Applicable to fermions (particles with half-integer spin).

\[ f_{FD}(\epsilon) = \frac{1}{e^{\beta(\epsilon - \mu)} + 1} \]

4. Bose–Einstein Distribution

Applicable to bosons (particles with integer spin).

\[ f_{BE}(\epsilon) = \frac{1}{e^{\beta(\epsilon - \mu)} - 1} \]

5. Comparison Table

Property Maxwell–Boltzmann Fermi–Dirac Bose–Einstein
Particle Type Classical particles Fermions Bosons
Spin Any Half-integer Integer
Distribution Function \( e^{-\beta(\epsilon-\mu)} \) \( \frac{1}{e^{\beta(\epsilon-\mu)}+1} \) \( \frac{1}{e^{\beta(\epsilon-\mu)}-1} \)
State Occupation No restriction Maximum 1 per state Unlimited
Quantum Effect Negligible Important at low T Important at low T
Low Temperature Behavior Classical limit fails Fermi energy dominates Bose condensation possible

6. Classical Limit

At high temperature and low density:

\[ e^{\beta(\epsilon - \mu)} \gg 1 \]

Both FD and BE distributions reduce to:

\[ f(\epsilon) \approx e^{-\beta(\epsilon - \mu)} \]
Thus, Maxwell–Boltzmann statistics is the classical limit of both Fermi–Dirac and Bose–Einstein statistics.

7. Important Result

The fundamental difference between FD and BE statistics arises due to the symmetry properties of the wave function:

This leads to completely different macroscopic behaviors such as degeneracy pressure and Bose–Einstein condensation.