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In Problem 7.28you found the density of states and the chemical potential for a two-dimensional Fermi gas. Calculate the heat capacity of this gas in the limit role="math" localid="1650099524353" kT≪εF· Also show that the heat capacity has the expected behavior when kT≫εF. Sketch the heat capacity as a function of temperature.

Short Answer

Expert verified

The heat capacity of the gas in the limit is CV=N(kπ)2T3εF.

The graph of heat capacity as a function of temperature is

Step by step solution

01

Given information

We have been given that the density of states and the chemical potential for a two-dimensional Fermi gas which we have found earlier in Problem 7.28isg(ε)=NεF.

We need to find the heat capacity of this gas in the limit kT≪εFand show that the heat capacity has the expected behavior when kT≫εF. Also we need to sketch the heat capacity as a function of temperature.

02

Simplify

The total energy is given by the following integral:

U=∫0∞εg(ε)n¯FD(ε)dε (Let this equation be (localid="1650103209259" 1))

We have found the energy density earlier in Problem 7.28such as

localid="1650102270353" g(ε)=NεF

Substitute the value of g(ε)in equation (localid="1650103517684" 1), we get:

U=NεF∫0∞εn¯FD(ε)dε

Integrating by parts, we get:

U=NεFε22n¯FD|0∞-NεF∫0∞ε22∂n¯FD∂εdε (Let this equation be (2))

If we substitute ε=0, the integral will become zero due to the dependence of the term on ε2and the first term vanishes.

The equation (2) reduces to :

U=-NεF∫0∞ε22∂n¯FD∂εdε (Let this equation be (3))

We know that n¯FD=1e(e-μ)kT+1

Taking derivative with respect to ε, we get:

localid="1650103912932" ∂n¯FD∂ε=∂1e(ε-μ)kT+1∂ε

∂n¯FD∂ε=-1kTe(ε-μ)kT(e(ε-μ)kT+1)2

Let (ε-μ)kT=x, then we can write as:

dx=dεkT

We also need to change the boundaries of integration, so:

ε→∞ x→∞

ε→0 x→-μkT

As kT≪μ, we can put -∞as the lower limit of integration.

The integral in equation (3) will become:

U=N2εF∫-∞∞ε2ex(ex+1)2dx (Let this equation be (localid="1650114310341" 4))

03

finding the values of integrals

Now expanding ε2about μusing Taylor series, we get:

ε2=μ2+2μ(ε-μ)x+(ε-μ)x2ε2=μ2+2μ(kTx)+(kTx)2

By substituting the value of in equation (4), we get three integrals say I1,I2,I3

The equation (4) will become:

U=N2εF[I1+I2+I3] (Let this equation be (5))

where,

I1=μ2∫-∞∞ex(ex+1)2dxI2=2kTμ∫-∞∞xex(ex+1)2dxI3=(kT)2∫-∞∞x2ex(ex+1)2dx

Simplifying the integrals I1,I2,I3, we get:

I1=μ2

The second integral is odd integral and the limits of integration are from to , so this integral is simply zero.

I2=0

I3=(kT)2Ï€23=(kTÏ€)23

Substitute the values of in equation (5), we get:

U=N2εFμ2+(kTπ)23

Let μ=εF, we get:

U=N2εFεF2+(kTπ)23U=NεF2+N(kTπ)26εF

The heat capacity is the partial derivative of with respect to the temperature, that is:

CV=∂U∂TCV=∂NεF2+N(kTπ)26εF∂TCV=N(kπ)2T3εF

04

Graph

The graph of the heat capacity as a function of temperature is linear, where the slope of the line is Slope=N(kπ)23εF.

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Most popular questions from this chapter

Sketch the heat capacity of copper as a function of temperature from 0to5K, showing the contributions of lattice vibrations and conduction electrons separately. At what temperature are these two contributions equal?

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Consider an isolated system of Nidentical fermions, inside a container where the allowed energy levels are nondegenerate and evenly spaced.* For instance, the fermions could be trapped in a one-dimensional harmonic oscillator potential. For simplicity, neglect the fact that fermions can have multiple spin orientations (or assume that they are all forced to have the same spin orientation). Then each energy level is either occupied or unoccupied, and any allowed system state can be represented by a column of dots, with a filled dot representing an occupied level and a hollow dot representing an unoccupied level. The lowest-energy system state has all levels below a certain point occupied, and all levels above that point unoccupied. Let ηbe the spacing between energy levels, and let be the number of energy units (each of size 11) in excess of the ground-state energy. Assume thatq<N. Figure 7 .8 shows all system states up to q=3.

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