The Sommerfeld expansion is an expansion in powers of kTεF, which is assumed to be small. In this section I kept all terms through order kTεF2, omitting higher-order terms. Show at each relevant step that the term proportional to localid="1650117451748" T3is zero, so that the next nonvanishing terms in the expansions forlocalid="1650117470867" μand localid="1650117476821" Uare proportional to localid="1650117458596" T4. (If you enjoy such things, you might try evaluating the localid="1650117464980" T4terms, possibly with the aid of a computer algebra program.)

Short Answer

Expert verified

At each step the term proportional to T3is zero and the next nonvanishing terms in the expansion for μand Uare proportional to T4in the proof of expressionU25g0μ52+5π28(kT)2μ12+7π4384(kT)4μ-32

Step by step solution

01

Given information

We have been given that the Sommerfeld expansion is an expansion in powers of kTεF, which is assumed to be small and we kept all terms through order kTεF2, omitting higher-order terms.

We need to show at each relevant step that the term proportional to role="math" localid="1650117659810" T3is zero, so that the next nonvanishing terms in the expansions forμandU are proportional toT4.

02

Simplify

The total energy given by the integral 7.54is:

U=0εg(ε)n¯FD(ε)dε

U=g00ε32n¯FD(ε)dε

Integrating by parts, we get:

U=25g0ε53n¯FD|0+25g00ε52n¯FDεdε (Let this equation be (1))

If we substitute ε=0, the integral becomes zero due to the dependence of the term on ε53and the first term vanishes.

On simplifying, the equation (1) becomes:

U=25g00ε52n¯FDεdε (Let this equation be (2))

We know that n¯FD=1e(ε-μ)kT+1

Taking derivative with respect to ε, we get:

n¯FDε=1e(ε-μ)kT+1ε

On simplifying, we get:

n¯FDε=1kTe(ε-μ)kTe(ε-μ)kT+12

Let localid="1650119493586" (ε-μ)kT=x, then we can write as :

dx=dεkT

Substitute dx,x,n¯FDεin equation (2), we get:
U=25g00ε521kTex(ex+1)2kTdx

U=25g00ε52ex(ex+1)2dx

03

Changing the limits of integration

We need to change the boundaries of integration, so:

εxε0x-μkT

As kTμ, so we can put -as the lower limit of integral, so the integral will become:

U=25g0-ε52ex(ex+1)2dx (Let this equation be (3))

Now by expanding the term ε52about μusing Taylor series, we get:

ε52=μ52+52(ε-μ)μ32+516(ε-μ)2μ12+5128(ε-μ)3μ-12+158(ε-μ)4μ-32...

Substitute ε-μ=kTx, we get:

ε52=μ52+52(kTx)μ32+158(kTx)2μ12+516(kTx)2μ-12+5128(kTx)2μ-32...

04

Finding the values of integrals 

Substitute the value of ε52in equation (3), we get three integral say I1,I2,I3:

U=25g0(I1+I2+I3+I4+I5) (Let this equation be (4))

where, I1=μ52-ex(ex+1)2dx

I2=52kTμ32-xex(ex+1)2dx

I3=158(kT)2μ12-x2ex(ex+1)2dx

I4=516(kT)3μ-12-x3ex(ex+1)2dx

I5=5128(kT)4μ-32-x4ex(ex+1)2dx

On simplifying I1,I2,I3,I4,I5, we get:

role="math" localid="1650601109788" I1=μ52I2=0I3=5π28(kT)2μ12I4=0I5=7π4384(kT)4μ-32

Substituting I1,I2,I3,I4,I5in equation (4), we get:

U25g0μ52+5π28(kT)2μ12+7π2384(kT)4μ-32

We have proved that the proportional term to T3is zero. We can also evaluate the further terms using computer algebra program, if wanted.

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Most popular questions from this chapter

In Section 6.5 I derived the useful relation F=-kTln(Z)between the Helmholtz free energy and the ordinary partition function. Use analogous argument to prove that ϕ=-kT×ln(Z^), where Z^ is the grand partition function and ϕis the grand free energy introduced in Problem 5.23.

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Evaluate the integral numerically.

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