- #1

- 74

- 1

[tex]

f(p) = \frac{1}{e^{\beta(\epsilon(p) - \mu)}+1} ,

[/tex]

where, in the Hartree-Fock approximation, we have

[tex]

\epsilon(p) = \frac{p^2}{2m} + n V(0) - \frac{1}{(2\pi \hbar)^3} \int d^3p' V(\textbf{p} - \textbf{p}' ) f(p').

[/tex]

Here, [tex]m[/tex] is the effective mass, [tex]n[/tex] is the particle density, [tex]V(0)[/tex] is the interaction potential [tex]V(q)[/tex] at zero momentum transfer. The potential may be assumed to depend only on the momentum transfer [tex]V(\textbf{p} - \textbf{p}' ) = V(| \textbf{p} - \textbf{p}' | ) = V(q)[/tex]. The F-D distribution [tex]f(p')[/tex] in the exchange term may be approximated with the non-interacting one. The chemical potential is determined by the condition (spin-1/2):

[tex]

n = \frac{2}{(2\pi \hbar)^3} \int d^3p f(p) = \frac{1}{\pi^2 \hbar^3} \int_0^\infty p^2 f(p) dp

[/tex]

Now, the right-hand side should somehow be expanded as a series in [tex]( k_B T/ \mu)^2[/tex], which can then be inverted to give [tex]\mu[/tex] as a function of [tex]T[/tex]. It seems that the Sommerfeld method used for a non-interacting system is not easy to use in this case. I know the result should be the following:

[tex]

\mu (T) = \mu_F (T) + n V(0) - \frac{1}{2} n \left[ F + G \frac{\pi^2}{12} \left( \frac{T}{T_F} \right)^2 \right] ,

[/tex]

where

[tex]

F = \frac{3}{2 k_F^3} \int_0^{2 k_F} k^2 \left( 1 - \frac{k}{2 k_F} \right) V(k) dk .

[/tex]

and

[tex]

G = 3 \left( V(2 k_F) - \frac{1}{4} \int_0^{2 k_F} \frac{k^3}{k_F^4} V(k) dk \right) .

[/tex]

The potential is now written as a function of the Fermi wave vector ([tex]p = \hbar k[/tex]). [tex]\mu_F (T)[/tex] is the chemical potential of a non-interacting Fermi gas. The zero temperature limit, i.e. [tex]F[/tex], is rather simple to derive.

Has anyone come across this problem or know any good references? I would really appreciate any assistance.