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Calculate the Fermi energy for copper, which has a density of8.9103kg/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=22m[3(2s+1)2NV]23 鈥︹. (1)

Here,

NNumber of oscillators

Planck's reduced constant

VVolume

sSpin

02

Given information from question and calculate the fermi energy 

Density of copper=8.9103kg/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=22m[3(2s+1)2NV]23=22m[3(2s+1)2DmA]23

Substitute9.11031kgfor mass of the electron (m),8.9103kg/m3for density of copper(D), 1.0551034J.sfor ,12forthe spin of the electron and 1.0551025kgformA.

role="math" localid="1658381931536" EF=2(1.0551034J.s)2(9.11031kg)[3(2(12)+1)2(8.9103kg/m3)(1.0551025kg)]23=1.1261018J

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

role="math" localid="1658381943480" EF=1.1261018J=(1.1261018J)(1eV1.6109J)=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

Equation (9-27) gives the density of states for a system of oscillators but ignores spin. The result, simply one state per energy change ofbetween levels, is incorrect if particles are allowed different spin states at each level, but modification to include spin is easy. From Chapter 8, we know that a particle of spinis allowedspin orientations, so the number of states at each level is simply multiplied by this factor. Thus,

D(E)=(2s+1)/h0.

(a) Using this density of states, the definitionNh0/(2s+1)=1, and

N=0N(E)D(E)dE

calculate the parameterin the Boltzmann distribution (9-31) and show that the distribution can thus be rewritten as

N(E)Boltz=kBT1eE/kBT

(b) Argue that ifkBT>>,the occupation number is much less than 1 for all E.

From elementary electrostatics the total electrostatic potential energy in a sphere of uniform charge Q and radius R is given by

U=3Q2540R

(a) What would be the energy per charge in a lead nucleus if it could be treated as 82 protons distributed uniformly throughout a sphere of radiusrole="math" localid="1659180305412" 710-15m

(b) How does this result fit with Exercise 87?

Copper has a density of8.9103kg/m3, and no photoelectrons are ejected from it if the wavelength of the incident light is greater than8.9103kg/m3(in the ultraviolet range). How deep is the well in which its conduction electrons--one per atom-are bound?

Consider the two-sided room, (a) Which is more likely to have an imbalance of five particles (i.e. Nk=12N+S,S): a room withN=20or a room withrole="math" localid="1658330090284" N=60? (Note: The total number of ways of distributing particles. the sum ofWNhNfrom 0 toN, is2N.) (b) Which is more likely to have an imbalance of5%(i.e. NR=12N+0.05N,)? (c) An average-size room is quite likely to have a trillion mote air molecules on one side than on the other, what may we say that precisely half will be on each side?

The Debye temperature of copper is 45K .

(a) Estimate its molar heat capacity at 100 K using the plot in Figure 9.33(b) .

(b) Determine its corresponding specific heat and compare it with the experimental value of 0.254闯/驳路碍.

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