Use the methods of this section to derive a formula, similar to equation2.21, for the multiplicity of an Einstein solid in the "low-temperature" limit,qN .

Short Answer

Expert verified

The formula of the Similar Equation

Ω=eNqq

Step by step solution

01

Solve the problem of solution

The number of microstates in an Einstein solid with Noscillators and qenergy quanta is:

Ω(q,N)=q+N-1q

For any macroscopic solid, both qandN are large numbers (on the order of Avogadro's number, orlocalid="1650382250464" 1023) so the factorials in Ωare very large numbers, not calculable on most computers. To get estimates ofΩwe can use Stirling's approximation for the factorials. The derivation of this approximation for the high temperature caseq>>N(lots more energy quanta than oscillators) is given in Schroeder's book, so at low temperature case we haveq<<N(lots more oscillators than energy quanta). Writing out the binomial coefficient:

Ω(q,N)=q+N-1q=(q+N-1)!q!(N-1)!(q+N)!q!N!

We can now take logarithms for both sides, we get,

ln(Ω)=ln(q+N)!q!N!

but, lnxy=ln(x)-ln(y)and ln(x)-ln(y)=ln(x)+ln(y), so:

ln(Ω)=\ln[(q+N)!]-\ln(q!)-\ln(N!)

use Stirling's approximation for the logarithm of a factorial:

ln(n!)nln(n)-n

02

The assumption of Equation

so equation (l) will become:

(Ω)=(q+N)ln(q+N)-(q+N)-qln(q)+q-Nln(N)+Nln(Ω)=(q+N)ln(q+N)-qln(q)-Nln(N)

If we now make the assumption thatq<<N, we get:

ln(Ω)=(q+N)lnN1+qN-qln(q)-Nln(N)ln(Ω)=(q+N)ln(N)+ln1+qN-qln(q)-Nln(N)

but forN>>q, we have,ln1+qN =\frac{q}{N}, so:

ln(Ω)=(q+N)ln(N)+qN-qln(q)-Nln(N)ln(Ω)=qln(N)+q2N+Nln(N)+q-qln(q)-Nln(N)ln(Ω)=(qln(N)-qln(q))+q2N+q

but,q\ln(N)-q\ln(q)qlnNq,= so:

ln(Ω)=qlnNq+q2N+q

03

Neglect the second term

but asq<<N, so we can neglect the second termq2N', so:

ln(Ω)=qlnNq+q

Exponentiating this equation gives the approximate value forΩ:

eln(Ω)=eqlnNq+q

Ω=elnNqq×eq

but,elnx=x, so:

Ω=Nqq×eq

Ω=eNqq

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Most popular questions from this chapter

Calculate the multiplicity of an Einstein solid with 30oscillators and 30units of energy. (Do not attempt to list all the microstates.)

Consider an ideal monatomic gas that lives in a two-dimensional universe ("flatland"), occupying an area Ainstead of a volume V. By following the same logic as above, find a formula for the multiplicity of this gas, analogous to equation 2.40.

Consider a two-state paramagnet with 1023elementary dipoles, with the total energy fixed at zero so that exactly half the dipoles point up and half point down.

(a) How many microstates are "accessible" to this system?

(b) Suppose that the microstate of this system changes a billion times per second. How many microstates will it explore in ten billion years (the age of the universe)?

(c) Is it correct to say that, if you wait long enough, a system will eventually be found in every "accessible" microstate? Explain your answer, and discuss the meaning of the word "accessible."

For each of the following irreversible processes, explain how you can tell that the total entropy of the universe has increased.
a Stirring salt into a pot of soup.
b Scrambling an egg.
c Humpty Dumpty having a great fall.
d A wave hitting a sand castle.
e Cutting down a tree.
fBurning gasoline in an automobile.

A black hole is a region of space where gravity is so strong that nothing, not even light, can escape. Throwing something into a black hole is therefore an irreversible process, at least in the everyday sense of the word. In fact, it is irreversible in the thermodynamic sense as well: Adding mass to a black hole increases the black hole's entropy. It turns out that there's no way to tell (at least from outside) what kind of matter has gone into making a black hole. Therefore, the entropy of a black hole must be greater than the entropy of any conceivable type of matter that could have been used to create it. Knowing this, it's not hard to estimate the entropy of a black hole.
aUse dimensional analysis to show that a black hole of mass Mshould have a radius of order GM/c2, where Gis Newton's gravitational constant and cis the speed of light. Calculate the approximate radius of a one-solar-mass black holeM=2×1030kg .
bIn the spirit of Problem 2.36, explain why the entropy of a black hole, in fundamental units, should be of the order of the maximum number of particles that could have been used to make it.

cTo make a black hole out of the maximum possible number of particles, you should use particles with the lowest possible energy: long-wavelength photons (or other massless particles). But the wavelength can't be any longer than the size of the black hole. By setting the total energy of the photons equal toMc2 , estimate the maximum number of photons that could be used to make a black hole of mass M. Aside from a factor of 8π2, your result should agree with the exact formula for the entropy of a black hole, obtained* through a much more difficult calculation:

Sb.h.=8π2GM2hck

d Calculate the entropy of a one-solar-mass black hole, and comment on the result.

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