Calculate the Fermi energy for copper, which has a density of8.9×103kg/m3and one conduction electron per atom. Is room temperature "cold"?

Short Answer

Expert verified

The Fermi energy for the copper is7.0eV . The room temperature is cold.

Step by step solution

01

Formula Used:

The energy of fermions at absolute zero temperature is known as Fermi energy. The mathematical equation for the Fermi energy is,

EF=π22m[3(2s+1)π2NV]23 ……. (1)

Here,

NNumber of oscillators

Planck's reduced constant

VVolume

sSpin

02

Given information from question and calculate the fermi energy 

Density of copper=8.9×103kg/m3

The NN in the equation (1) can be rewritten as the mass per unit volume over the mass per atom, or the bulk density D over the atomic mass:

role="math" localid="1658381923377" EF=π22m[3(2s+1)π2NV]23=π22m[3(2s+1)π2DmA]23

Substitute9.1×1031kgfor mass of the electron (m),8.9×103kg/m3for density of copper(D), 1.055×1034J.sfor ,12forthe spin of the electron and 1.055×1025kgformA.

role="math" localid="1658381931536" EF=π2(1.055×1034J.s)2(9.1×1031kg)[3(2(12)+1)π2(8.9×103kg/m3)(1.055×1025kg)]23=1.126×1018J

Convert the unit for Fermi energy for copper energy from JtoeV .

role="math" localid="1658381943480" EF=1.126×1018J=(1.126×1018J)(1eV1.6×109J)=7.04eV

Therefore, the Fermi energy for the copper is7.04eV .

Since the energy that a particle at room temperature would have been 0.04eV(from 32kBT), as opposed to the Fermi energy of 7.0eV, room temperature would be considered cold in comparison.

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Most popular questions from this chapter

The electrons’ contribution to the heat capacity of a metal is small and goes to 0as T0. We might try to calculate it via the total internal energy, localid="1660131882505" U=EN(E)D(E)dE, but it is one of those integrals impossible to do in closed form, and localid="1660131274621" N(E)FDis the culprit. Still, we can explain why the heat capacity should go to zero and obtain a rough value.

(a) Starting withN(E)FDexpressed as in equation (34), show that the slope N(E)FDdEatE=EFis-1(4kBT).

(b) Based on part (a), the accompanying figure is a good approximation to N(E)FDwhen Tis small. In a normal gas, such as air, whenTis raised a little, all molecules, on average, gain a little energy, proportional to kBT. Thus, the internal energy Uincreases linearly with T, and the heat capacity, UT, is roughly constant. Argue on the basis of the figure that in this fermion gas, as the temperature increases from 0to a small value T, while some particles gain energy of roughly kBT, not all do, and the number doing so is also roughly proportional to localid="1660131824460" T. What effect does this have on the heat capacity?

(c)Viewing the total energy increase as simply U= (number of particles whose energy increases) (energy change per particle) and assuming the density of states is simply a constant Dover the entire range of particle energies, show that the heat capacity under these lowest-temperature conditions should be proportional to kBREFT. (Trying to be more precise is not really worthwhile, for the proportionality constant is subject to several corrections from effects we ignore).

Show that equation (9- 16) follows from (9-15) and (9- 10).

Exercise 54 calculates the three oscillator distributions'E=0values in the special case wherekBTis15ξ. Using a very common approximation technique. show that in the more general low-temperature limit,kBTε,theoccupation numbers becomeδ/kBT,e5/kBT, and 1, for the distinguishable. boson. and fermion cases, respectively. Comment on these results. (Note: Although we assume thatkBTNω0/(2s+1). we also still assume that levels are closely spaced-that is kBhω0.),

Copper has one conduction electron per atom and a density of8.9×103kg/m3. By the criteria of equation(943), show that at room temperature(300K), the conduction electron gas must be treated as a quantum gas of indistinguishable particles.

Determine the density of statesD(E)for a 2D infinite well (ignoring spin) in whichEnx,ny=(nx2+ny2)π222mL2

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