Problems and Solutions on Thermodynamics and Statistical Mechanics

(Ann) #1
178 Problem8 El Solution.$ on Thermodynamics d Statistical Mechanic8

Solution:
(a) Classical Maxwell-Boltzmann statistics is appropriate because
h2 3/2
nX 3P =-.(-----) x 3 x lor6 << 1.
kT 21rmkT
(b) Fermi-Dirac statistics is appropriate because electrons are Fermions
and the Fermi energy of the electron gas in copper is about 1 eV which
is equivalent to a high temperature of 104K. At room temperature (low
temperature), the electron gas is highly degenerate.


(c) Classical Maxwell-Boltzmann statistics is appropriate because at
room temperature the electrons and holes do not have sufficient average
energy to jump over the 1 eV band-gap in appreciable numbers.


2017
Show that X = exp(p/kT) = nVQ for an ideal gas, valid where X << 1;
here p is the chemical potential, n is the gas density and
VQ = (h’/21rmkT)~/~
is the quantum volume. Even if you cannot prove this, this result will be
useful in other problems.
(UC, Berkeley)
Solution:
In the approximation X << 1, Fermi-Dirac and Bose-Einstein statistics
both tend to Maxwell-Boltzmann statistics:

The density of states of an ideal gas (spin states excluded) is
2lr
h3

D(+ = -(2m)3/2fide.


Therefore,

That is, X = nVQ.

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