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Fill in the steps to derive equations 7.112and7.117.

Short Answer

Expert verified

The derived equations are U=9NkT4TD30xmaxx3ex-1dxandCV=3π21(kTD)36Nπk4T30xmaxx4ex(ex-1)2dx.

Step by step solution

01

Given Information

We need to fill in the steps to derive equations.

02

Simplify

The total thermal energy equals the sum of planck distribution all over the modes nx,nyandnzmultiplied by the energy ofeach mode, and sum is multiplied by factor of 3 because we have three polarization modes in crystal, that is:

role="math" localid="1650022039736" U=3nxnynzεn¯P1(ε)=nxnynzεn¯P1(ε)

but,

n¯P1(ε)=1eε/kT-1

consider we have a cubic box with volume of V and side width of L, the allowed energy for the photon is:

ε=hcsn2L

where csis the speed of sound in the crystal substitute into the above equation to get:

U=3hcs2Lnx,ny,nznehcsn/2LkT-1

now we need to change the sum to an integral in spherical coordinates, by multiplying this by the spherical integration factor n2sin(θ), so we get:

U=3hcs2L0π/2dϕ0π/2sin(θ)dθ0nmaxn3ehcsn/2LkT-1dn

the first two integrals are easy to evalute, and they give a factor ofπ/2,so:

now let,U=3πhcs4L0nmaxn3ehcsn/2LkT-1dnx=hcsn2LkTdx=hcs2LkTdn

thus,

U=3πhcs4L2LkThcs30nmaxx3ex-1dxU=3π22Lhcs(kT)40xmaxx3ex-1dx

03

simplify

We need to change the limits of the integral, the lover limit will stay the same while the upper limit is:

xmax=hcsnmax2LkT

also we can write xmaxas:

xmax=TDT=hcsnmax2LkT=hcs2LkT6Nπ1/3

TD=hcs2Lk6Nπ1/3

TD3=1k3hcs2L36Nπ2Lhcs3=1(kTD)36Nπ

substitute into (2) to get:

U=3π21(kTD)36Nπ(kT)40xmaxx3ex-1dxU=9NkT4TD30xmaxx3ex-1dx

04

Simplify

the heat capacity at volume equals the partial derivative of the total energy with respect to the temperature, that is:

CV=aUaT

substitute form(1) to getCV=9NkTTD30xmaxx3ex(ex-1)2dx

CV=3πhcs4L0nmaxUTn3ehcsn/2LkT-1dn

CV=3πhcs4L0nmaxhcsn2LkT2n3ehcsn/2LkT(ehcsn/2LkT-1)2dn

CV=3π2hcs2L21kT20nmaxn4ehcsn/2LkT(ehcsn/2LkT-1)dn

now let,

x=hcsn2LkTdx=hcs2LkTdn

thus,

CV=3π2hcs2L21kT22LkThcs50xmaxx4ex(ex-1)2dx

CV=3π22Lhcs3k4T30xmaxx4ex(ex-1)2dx

CV=3π21(kTD)36Nπk4T30xmaxx4ex(ex-1)2dx

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Most popular questions from this chapter

Consider a free Fermi gas in two dimensions, confined to a square area A=L2

(a) Find the Fermi energy (in terms of Nand A), and show that the average energy of the particles is F2.

(b) Derive a formula for the density of states. You should find that it is a constant, independent of .

(c) Explain how the chemical potential of this system should behave as a function of temperature, both when role="math" localid="1650186338941" kTFand when Tis much higher.

(d) Because gis a constant for this system, it is possible to carry out the integral 7.53 for the number of particles analytically. Do so, and solve for μas a function of N. Show that the resulting formula has the expected qualitative behavior.

(e) Show that in the high-temperature limit, kTF, the chemical potential of this system is the same as that of an ordinary ideal gas.

In the text I claimed that the universe was filled with ionised gas until its temperature cooled to about 3000 K. To see why, assume that the universe contains only photons and hydrogen atoms, with a constant ratio of 109 photons per hydrogen atom. Calculate and plot the fraction of atoms that were ionised as a function of temperature, for temperatures between 0 and 6000 K. How does the result change if the ratio of photons to atoms is 108 or 1010? (Hint: Write everything in terms of dimensionless variables such as t = kT/I, where I is the ionisation energy of hydrogen.)

Explain in some detail why the three graphs in Figure 7.28 all intercept the vertical axis in about the same place, whereas their slopes differ considerably.

Consider a degenerate electron gas in which essentially all of the electrons are highly relativistic ϵmc2so that their energies are ϵ=pc(where p is the magnitude of the momentum vector).

(a) Modify the derivation given above to show that for a relativistic electron gas at zero temperature, the chemical potential (or Fermi energy) is given by =

μ=hc(3N/8πV)1/3

(b) Find a formula for the total energy of this system in terms of N and μ.

Starting from the formula for CV derived in Problem 7.70(b), calculate the entropy, Helmholtz free energy, and pressure of a Bose gas for T<Tc. Notice that the pressure is independent of volume; how can this be the case?

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