04.08.2013 Views

Statistical Mechanics - Physics at Oregon State University

Statistical Mechanics - Physics at Oregon State University

Statistical Mechanics - Physics at Oregon State University

SHOW MORE
SHOW LESS

You also want an ePaper? Increase the reach of your titles

YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.

2.1. INTRODUCTION. 25<br />

PS(s) ∝ gR(U0 − ɛs) (2.4)<br />

Therefore the r<strong>at</strong>io of the probabilities of finding the system in st<strong>at</strong>e 1 and 2 is<br />

PS(1)<br />

PS(2) = gR(U0 − ɛ1) 1<br />

k (SR(U0−ɛ1)−SR(U0−ɛ2))<br />

= e B<br />

gR(U0 − ɛ2)<br />

Because the reservoir is very large, the difference between the entropies is<br />

SR(U0 − ɛ1) − SR(U0 − ɛ2) ≈ −(ɛ1 − ɛ2)<br />

<br />

∂S<br />

(U0) = −<br />

∂U V,N<br />

ɛ1 − ɛ2<br />

TR<br />

(2.5)<br />

(2.6)<br />

The reservoir and the system are in thermal equilibrium, and have the same<br />

temper<strong>at</strong>ure T. We drop the subscript on the temper<strong>at</strong>ure because is is the same<br />

for both system and reservoir. We find<br />

or in general<br />

PS(1)<br />

PS(2) = e− ɛ 1 −ɛ 2<br />

k B T (2.7)<br />

ɛs − k PS(s) ∝ e B T (2.8)<br />

This is the well-known Boltzmann factor. The only reference to the reservoir<br />

is via the temper<strong>at</strong>ure T, no other details of the reservoir are involved.<br />

Normaliz<strong>at</strong>ion requires P (s) = 1 and hence we define<br />

Z(T ) = <br />

s<br />

ɛs − k e B T (2.9)<br />

PS(s) = 1 ɛs<br />

k e− B T (2.10)<br />

Z<br />

The probability PS(s) depends on the temper<strong>at</strong>ure T of the system, and<br />

although there is no explicit reference to the reservoir there is still an implicit<br />

reservoir through T. Specifying T requires contact with an outside reservoir.<br />

Also, the probability only depends on the energy ɛs of the st<strong>at</strong>e and not on<br />

any other property of this st<strong>at</strong>e. All different st<strong>at</strong>es with the same energy have<br />

the same probability. The quantity Z(T ) is called the partition function. We<br />

will see l<strong>at</strong>er th<strong>at</strong> for a description of a system <strong>at</strong> temper<strong>at</strong>ure T the partition<br />

function is all we need to know. The probability distribution PS(s) of this form<br />

is called the Boltzmann distribution. The partition function is also a function of<br />

volume and number of particles. The dependence on all extensive st<strong>at</strong>e variables,<br />

excluding the entropy, is via the energy of the quantum st<strong>at</strong>es. In general, the<br />

energy eigenvalues ɛs are functions of the volume V and the number of particles<br />

N. Note th<strong>at</strong> the quantum st<strong>at</strong>es we consider here are N-particle quantum st<strong>at</strong>es.<br />

The energy ɛs(V, N) is the energy of a collective st<strong>at</strong>e and is not equal to the<br />

energy of a given particle!

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!