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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)

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