Statistical Mechanics - Physics at Oregon State University
Statistical Mechanics - Physics at Oregon State University
Statistical Mechanics - Physics at Oregon State University
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78 CHAPTER 4. STATISTICS OF INDEPENDENT PARTICLES.<br />
In our discussion of the ideal gas we have assumed th<strong>at</strong> the orbitals are<br />
characterized by three quantum numbers nx, ny, and nz. These three quantum<br />
numbers describe the motion of the center of mass of the particle, but did not<br />
include any internal degrees of freedom. Therefore, the previous formulas only<br />
are valid for a gas of mono-<strong>at</strong>omic molecules. A gas of poly-<strong>at</strong>omic molecules is<br />
easily tre<strong>at</strong>ed if we assume th<strong>at</strong> the energy associ<strong>at</strong>ed with the internal degrees<br />
of freedom does not depend on (1) the presence of other particles and (2) the<br />
motion of the center of mass. Hence the rot<strong>at</strong>ion of a di<strong>at</strong>omic molecule is not<br />
hindered by neighboring molecules or changed by its own motion. In th<strong>at</strong> case<br />
we can write, using int for the collective internal degrees of freedom:<br />
ɛ(nx, ny, nz, int) = 2<br />
<br />
π<br />
2 (n<br />
2M L<br />
2 x + n 2 y + n 2 z) + ɛint (4.43)<br />
Then internal degrees of freedom represent the rot<strong>at</strong>ional quantum numbers<br />
(of which there are <strong>at</strong> most three) and the vibr<strong>at</strong>ional quantum numbers. If<br />
we have a molecule with N <strong>at</strong>oms, there are 3N internal degrees of freedom.<br />
Three are used for the center of mass, r for the rot<strong>at</strong>ions (r is 2 or 3) and hence<br />
3(N − 1) − r for the vibr<strong>at</strong>ional st<strong>at</strong>e.<br />
Changes in the partition function.<br />
In the classical regime µ ≪ −kBT and hence λ = e µ<br />
k B T ≪ 1. In the partition<br />
function for a given orbital terms with λ 2 and higher powers can be neglected<br />
for bosons and in all cases we find<br />
Zo(T, µ, V ) = 1 + λ <br />
where the internal partition function is defined by<br />
int<br />
Zint(T ) = <br />
e − ɛo+ɛint ɛo<br />
kB T − k = 1 + λZinte B T (4.44)<br />
int<br />
e − ɛ int<br />
k B T (4.45)<br />
The average number of particles in orbital o, independent of its internal<br />
st<strong>at</strong>e, is therefore given by<br />
< no >= <br />
int<br />
λe − ɛ int<br />
k B T e − ɛo<br />
k B T<br />
1 + λ <br />
int e− ɛ int<br />
k B T e − ɛo<br />
k B T<br />
ɛo − k ≈ λZinte B T (4.46)<br />
where we used the fact th<strong>at</strong> the denomin<strong>at</strong>or is approxim<strong>at</strong>ely equal to one<br />
because λ is very small. Hence in the Boltzmann distribution function we have<br />
to replace λ by λZint(T ) and we find<br />
N = λZint(T )nQ(T )V (4.47)<br />
<br />
<br />
n<br />
µ = kBT log( ) − log(Zint)<br />
nQ(T )<br />
(4.48)