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Fermi Distribution Functions

Fermi-Dirac (F-D) Statistics Derivation

The following derivation covers the thermodynamic probability and the occupation index for fermions, which are indistinguishable particles that obey the Pauli exclusion principle.

1. Thermodynamic Probability (W)

Consider $n_i$ fermions to be distributed among $g_i$ energy cells. Due to the Pauli Exclusion Principle, each cell can hold at most one fermion.

The total number of ways for one energy level is given by:
W_i = g_i(g_i-1)(g_i-2)...(g_i - n_i + 1) = g_i!/ (g_i - n_i)!

Since fermions are indistinguishable, we divide by $n_i!$:

W_i = g_i! / [n_i! (g_i - n_i)!]

The total thermodynamic probability for the entire system is the product across all energy levels:

W = Π [g_i! / (n_i! (g_i - n_i)!)]

2. Occupation Index (n_i / g_i)

To find the distribution in equilibrium, we maximize $\ln W$ subject to the constraints of constant total number of particles ($\sum n_i = N$) and constant total energy ($\sum n_i E_i = U$)

Step A: Logarithm and Differentiation

Taking the natural logarithm and applying Stirling's Approximation

ln W = Σ [ln g_i! - ln n_i! - ln(g_i - n_i)!]

Differentiating for the maximum ($d \ln W = 0$) leads to

Σ ln[(g_i - n_i) / n_i] dn_i = 0

Step B: Lagrange Multipliers

Using multipliers $\alpha$ and $\beta$ for the constraints[cite: 421, 423]:

ln[(g_i - n_i) / n_i] = α + β E_i

Exponentiating both sides:

(g_i - n_i) / n_i = e^(α + β E_i)

(g_i / n_i) - 1 = e^(α + β E_i)

Final Result: The Occupation Index

The average number of particles per state (occupation index) is:

f(E_i) = n_i / g_i = 1 / [e^(α + β E_i) + 1]

\[\begin{align} {{W}_{1}}&={{g}_{1}}\times \left( {{g}_{1}}-1 \right)\times \left( {{g}_{1}}-2 \right).....\left( {{g}_{1}}-\left( {{n}_{1}}-1 \right) \right) \\ & ={{g}_{1}}\left( {{g}_{1}}-1 \right)\left( {{g}_{1}}-2 \right).....\left( {{g}_{1}}-{{n}_{1}}+1 \right) \\ & =\frac{{{g}_{1}}\left( {{g}_{1}}-1 \right)\left( {{g}_{1}}-2 \right).....\left( {{g}_{1}}-{{n}_{1}}+1 \right)\left( {{g}_{1}}-{{n}_{1}} \right)\left( {{g}_{1}}-{{n}_{1}}-1 \right)....3\times 2\times 1}{\left( {{g}_{1}}-{{n}_{1}} \right)\left( {{g}_{1}}-{{n}_{1}}-1 \right)....3\times 2\times 1} \\ & =\frac{{{g}_{1}}!}{\left( {{g}_{1}}-{{n}_{1}} \right)!} \\ & \Rightarrow {{W}_{2}}=\frac{{{g}_{2}}!}{\left( {{g}_{2}}-{{n}_{2}} \right)!},{{W}_{3}}=\frac{{{g}_{3}}!}{\left( {{g}_{3}}-{{n}_{3}} \right)!}... \\ & \Rightarrow W={{W}_{1}}{{W}_{2}}{{W}_{3}}.... \\ & =\frac{{{g}_{1}}!}{\left( {{g}_{1}}-{{n}_{1}} \right)!}\frac{{{g}_{2}}!}{\left( {{g}_{2}}-{{n}_{2}} \right)!}\frac{{{g}_{3}}!}{\left( {{g}_{3}}-{{n}_{3}} \right)!}... \\ & =\prod\limits_{i=1}^{i=n}{\frac{{{g}_{i}}!}{\left( {{g}_{i}}-{{n}_{i}} \right)!}} \\ \end{align}\]
\begin{align} \ln W&=\ln \prod\limits_{i=1}^{i=n}{\frac{{{g}_{i}}!}{{{n}_{i}}!\left( {{g}_{i}}-{{n}_{i}} \right)!}} \\ & =\sum{\ln {{g}_{i}}!}-\sum{\ln \left( {{n}_{i}}!\left( {{g}_{i}}-{{n}_{i}} \right)! \right)} \\ & =\sum{\ln {{g}_{i}}!}-\sum{\ln {{n}_{i}}!}-\sum{\ln \left( {{g}_{i}}-{{n}_{i}} \right)!} \\ & =\sum{\ln {{g}_{i}}!}-\sum{{{n}_{i}}\left( \ln {{n}_{i}}-1 \right)}-\sum{\left( {{g}_{i}}-{{n}_{i}} \right)\left( \ln \left( {{g}_{i}}-{{n}_{i}} \right)-1 \right)} \\ & =\sum{\ln {{g}_{i}}!}-\sum{{{n}_{i}}\left( \ln {{n}_{i}} \right)}+\sum{{{n}_{i}}}-\sum{\left( {{g}_{i}}-{{n}_{i}} \right)\ln \left( {{g}_{i}}-{{n}_{i}} \right)}+\sum{\left( {{g}_{i}}-{{n}_{i}} \right)} \\ & =\sum{\ln {{g}_{i}}!}-\sum{{{n}_{i}}\left( \ln {{n}_{i}} \right)}-\sum{\left( {{g}_{i}}-{{n}_{i}} \right)\ln \left( {{g}_{i}}-{{n}_{i}} \right)}+\sum{{{g}_{i}}} \\ & \Rightarrow d\left( \ln W \right)=0-\sum{d{{n}_{i}}\left( \ln {{n}_{i}} \right)-}\sum{{{n}_{i}}\left( \frac{1}{{{n}_{i}}} \right)}d{{n}_{i}}-\sum{\left( -d{{n}_{i}} \right)\ln \left( {{g}_{i}}-{{n}_{i}} \right)}-\sum{\left( {{g}_{i}}-{{n}_{i}} \right)\frac{1}{\left( {{g}_{i}}-{{n}_{i}} \right)}}\left( -d{{n}_{i}} \right)+0 \\ & =-\sum{d{{n}_{i}}\left( \ln {{n}_{i}} \right)-}\sum{d{{n}_{i}}}+\sum{\ln \left( {{g}_{i}}-{{n}_{i}} \right)d{{n}_{i}}}+\sum{d{{n}_{i}}} \\ & =\sum{\ln \left( {{g}_{i}}-{{n}_{i}} \right)d{{n}_{i}}}-\sum{\left( \ln {{n}_{i}} \right)d{{n}_{i}}} \\ & =\sum{\ln \frac{\left( {{g}_{i}}-{{n}_{i}} \right)}{{{n}_{i}}}d{{n}_{i}}} \\ & \Rightarrow \sum{\ln \frac{\left( {{g}_{i}}-{{n}_{i}} \right)}{{{n}_{i}}}d{{n}_{i}}}=0\left( \because d\left( \ln W \right)=0 \right) \\ & U=\sum{{{n}_{i}}{{E}_{i}}} \\ & N=\sum{{{n}_{i}}} \\ & \Rightarrow dU+dN=\beta \sum{d{{n}_{i}}{{E}_{i}}}+\alpha \sum{d{{n}_{i}}} \\ & \Rightarrow \beta \sum{d{{n}_{i}}{{E}_{i}}}+\alpha \sum{d{{n}_{i}}}=0 \\ & \Rightarrow \sum{\left( \beta {{E}_{i}}+\alpha \right)d{{n}_{i}}}=0 \\ & \Rightarrow \sum{\ln \frac{\left( {{g}_{i}}-{{n}_{i}} \right)}{{{n}_{i}}}d{{n}_{i}}}=\sum{\left( \beta {{E}_{i}}+\alpha \right)d{{n}_{i}}} \\ & \Rightarrow \ln \frac{\left( {{g}_{i}}-{{n}_{i}} \right)}{{{n}_{i}}}=\left( \beta {{E}_{i}}+\alpha \right) \\ & \Rightarrow \frac{\left( {{g}_{i}}-{{n}_{i}} \right)}{{{n}_{i}}}={{e}^{\left( \beta {{E}_{i}}+\alpha \right)}} \\ & \Rightarrow \frac{{{g}_{i}}}{{{n}_{i}}}-1={{e}^{\alpha +\beta {{E}_{i}}}} \\ & \Rightarrow \frac{{{g}_{i}}}{{{n}_{i}}}=1+{{e}^{\alpha +\beta {{E}_{i}}}} \\ & \Rightarrow \frac{{{n}_{i}}}{{{g}_{i}}}=\frac{1}{{{e}^{\alpha +\beta {{E}_{i}}}}+1} \\ & \Rightarrow f\left( {{E}_{i}} \right)=\frac{1}{{{e}^{\alpha +\beta {{E}_{i}}}}+1} \\ \end{align}

Fermi–Dirac Statistics – MCQ Quiz

Fermi–Dirac statistics applies to particles called:





Fermions obey which principle?





The Fermi–Dirac distribution function is:





At absolute zero temperature, the occupation probability below Fermi energy is:





Fermi energy is defined at:





Maximum number of fermions in a single quantum state is:





The chemical potential at T = 0 K is equal to:





At high temperature and low density, Fermi–Dirac statistics reduces to:





The spin of fermions is:





Electrons in metals follow:





At ε = μ, the Fermi–Dirac distribution value is:





Degeneracy pressure arises due to:





Fermi temperature is defined as:


Fermi–Dirac distribution is symmetric about:





White dwarf stars are supported by degeneracy of: