Advanced Solid State Physics

(Axel Boer) #1

where every odd term is zero (x,x^3 ,x^5 ) and the other ones are just numbers. If you put in these
terms you get


n=

∫∞

−∞

H(E)f(E)dE=K(μ) +
π^2
6

(kBT)^2
dH(E)
dE E=μ

+

7 π^4
360

(kBT)^4
d^3 H(E)
dE^3 E=μ

+...

Sommerfeld Expansion: Chemical Potential 3D
It is possible to get the chemical potential out of the Sommerfeld expansion. IfH(E) =D(E), which
you get out of the dispersion relationship, you can getK(E)which is just the integral ofH(E)over
all energies. You get the non-linear relationship of theμand theT (EF as the fermi energy):


n=
nμ^1 /^2
E^3 F/^2

+

π^2
8
(kBT)^2
nμ−^1 /^2
E^3 F/^2

+...

Dividing both sides byngives:


1 =

μ^1 /^2
EF^3 /^2

+

π^2
8

(kBT)^2
μ−^1 /^2
EF^3 /^2

+...

Sommerfeld Expansion: Internal energy
In this caseH(E) =D(E)E. So we get the expression for the internal energy:


u=

∫∞

−∞

H(E)f(E)dE=
3 n
5 EF^3 /^2

μ^3 /^2 +
3 π^2
8

(kBT)^2
n
E^3 F/^2

μ^1 /^2

Sommerfeld Expansion: Electronic specific heat
If you differentiate the internal energy once you get the specific heatcV. So you see that the specific
heat is linear with the temperature.


cV=
du
dT

=

3 π^2
4

(kBT)
n
EF^3 /^2

μ^1 /^2 +....

If you take a metal and measure the specific heat at a certain temperatureT, some of the energy goes
into the electrons (∝T) and some into the phonons (∝T^3 ), because both are present in a metal:


cV=γT+AT^3
C
T is plotted versusT

(^2) to get a line (see fig. 21). The slope of the line is the phonon constantAand
the interception with the y-axis givesγ, the constant for the electrons.
Typically metals are given aneffective massm∗, which was reasonable when comparing the calcu-
lated free electron case (massme,γ) with the results measured (γobserved) (The effective mass is a way
to parameterize a system - interaction was neglected). What was really done with this was specifying
a derivative of the Sommerfeld expansion. So because of history we are talking about effective mass,
but we mean this derivative in the Sommerfeld expansion.
m∗
me


=

γobserved
γ

and m∗=

2

9

dH
dEE=μ

·me
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