05.04.2016 Views

Modern Engineering Thermodynamics

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

750 CHAPTER 18: Introduction to Statistical <strong>Thermodynamics</strong><br />

Table 18.7 Formula for Computing the Number of Microstates in the ith Macrostate<br />

for Various Statistical Models<br />

Model<br />

Maxwell-Boltzmann<br />

Fermi-Dirac<br />

Bose-Einstein<br />

Note: Here, Z = ∑g i expð−ε i /kT<br />

Number of Microstates per<br />

Macrostate, W<br />

N!<br />

g<br />

∏ i<br />

N<br />

i i !<br />

∏<br />

i<br />

g i !<br />

N i !ðg i − N i Þ!<br />

ðg i + N i − 1Þ!<br />

∏<br />

N<br />

i i !ðg i − 1Þ!<br />

Most Probable Distribution (N i ) mp<br />

<br />

N<br />

Z<br />

gi exp − ε <br />

i<br />

kT<br />

h <br />

g i B exp ε i −1<br />

i<br />

kT<br />

+ 1<br />

h <br />

g i B exp ε <br />

i<br />

kT<br />

− 1<br />

Þ = partition function, and B = expð− μ/kTÞ, where μ is the molar chemical potential.<br />

i −1<br />

The problem we now face is that the total entropy S of a system is an additive property whereas W mp is not. In<br />

the probability mathematics presented earlier, we found that the probability that independent events A and B<br />

simultaneously occur is P (A and B) = P AB = P A P B , and since W mp is related to mathematical probability through<br />

Eq. (18.38), we can write<br />

but<br />

Therefore, we must find a function f such that<br />

WAand ð BÞ = W A W B<br />

SAand ð BÞ = S A + S B<br />

SAand ð BÞ = fðW A Þ+ fðW B Þ = fWAand ½ ð BÞŠ = fðW A W B Þ<br />

The only general function that satisfies this relation is the logarithm, since<br />

ln W A + ln W B = ln W A W B<br />

Therefore, we choose to set S proportional to ln W mp . It can be shown that the constant of proportionality in<br />

this relation is just Boltzmann’s constant k, so we end up with the following entropy-probability relation:<br />

Thus, we see that entropy is a measure of the molecular order within a system.<br />

S = k ln W mp (18.40)<br />

18.10 MAXWELL-BOLTZMANN GASES<br />

To limit the algebraic complexity of the resulting property formula, we restrict our attention to the Maxwell-<br />

Boltzmann model. It can be shown that, for Maxwell-Boltzmann gases with N ≫ 1,<br />

<br />

u = RT 2 ∂ ln Z <br />

(18.41)<br />

∂T<br />

and<br />

where<br />

h = u + RT (18.42)<br />

Z = ∑g i expð−ε i /kTÞ<br />

Z is called the partition function of the system and g i is the degeneracy of the ith energy level ε i . At high temperatures,<br />

the number of quantum states (or degeneracy levels g i ) available at any energy level is much larger than<br />

the number of particles N i in that energy level, or<br />

g i<br />

N i<br />

≫ 1

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

Saved successfully!

Ooh no, something went wrong!