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Consider two single-particle states, A and B, in a system of fermions, where ϵA=μ-xand ϵB=μ+x; that is, level A lies below μ by the same amount that level B lies above μ. Prove that the probability of level B being occupied is the same as the probability of level A being unoccupied. In other words, the Fermi-Dirac distribution is "symmetrical" about the point where ϵ=μ.

Short Answer

Expert verified

It is proved that the probability of level B being occupied is the same as the probability of level A being unoccupied.

Step by step solution

01

Step 1. Givne Information

We are given that the level A lies below μ by the same amount that level B lies above μ.

We have to prove thatthe probability of level B being occupied is the same as the probability of level A being unoccupied.

02

Step 2. Fermi-Dirac distribution

Using the Fermi-Dirac distribution to calculate the probability of state B being occupied as follows:

P(Boccupied)=1e4ε0-μUT+1

Here, εBis the energy for the occupled state of B,μ is the chemical potential, k is the Boltzmann's constant, and T is the temperature.

The energy for the occupied state of B is,

εB=μ+x

Substitute μ+xfor εB in the equation and simplifying, we get

P(Boccupied)=1et(μ+x-μ)kT+1=1exkT+1

03

Step 3. Probability of state A

The probability of state A being unoccupied is as follows,

P(AUnoccupied)=1-P(Aoccupied)

Using the Fermi-Dirac distribution, the probability of state A being occupied is as follows,

P(Aoccupied)=1e+εA-μNT+1

Where εA is the energy for the occupied state of A.

Substituting the values, we get

P(AUnoccupied)=1-1e+εA-μkT

The energy for the occupied state of A is,

εA=μ-x

Substituting the values, we get

P(AUnoccupied)=1-1e+(μ-x-μ)kT+1=1-1e-xkT+1=e-xkTe-xkT+1=11+exkT

04

Step 4. Proving the Probability

Now, substituting P(Aunoccupied)=11+exkTin the equation,

P(Boccupied)=1exkT+1, we get

P(Boccupied)=P(Aunoccupied)

Hence, the probability of level B being occupied is same as the probability of level A being unoccupied or the Fermi-Dirac distribution being symmetrical about the point where ε=μ.

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Most popular questions from this chapter

It's not obvious from Figure 7.19 how the Planck spectrum changes as a function of temperature. To examine the temperature dependence, make a quantitative plot of the functionu(ϵ) for T = 3000 K and T = 6000 K (both on the same graph). Label the horizontal axis in electron-volts.

Change variables in equation 7.83 to λ=hc/ϵ and thus derive a formula for the photon spectrum as a function of wavelength. Plot this spectrum, and find a numerical formula for the wavelength where the spectrum peaks, in terms of hc/kT. Explain why the peak does not occur at hc/(2.82kT).

Use the results of this section to estimate the contribution of conduction electrons to the heat capacity of one mole of copper at room temperature. How does this contribution compare to that of lattice vibrations, assuming that these are not frozen out? (The electronic contribution has been measured at low temperatures, and turns out to be about40% more than predicted by the free electron model used here.)

Consider a degenerate electron gas in which essentially all of the electrons are highly relativistic ϵ≫mc2so 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.

Prove that the peak of the Planck spectrum is at x = 2.82.

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