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The density of copper is8.96g/cm3,and its atomic weight is63.5g/mole

(a) Calculate the Fermi energy for copper (Equation 5.43). Assume d = 1, and give your answer in electron volts.

EF=ħ22m3ρπ22/3 (5.43).

(b) What is the corresponding electron velocity? Hint: SetEF=1/2mv2Is it safe to assume the electrons in copper are nonrelativistic?

(c) At what temperature would the characteristic thermal energyrole="math" localid="1656065555994" (kBT,wherekBkBis the Boltzmann constant and T is the Kelvin temperature) equal the Fermi energy, for copper? Comment: This is called the Fermi temperature,TF

. As long as the actual temperature is substantially below the Fermi temperature, the material can be regarded as “cold,” with most of the electrons in the lowest accessible state. Since the melting point of copper is 1356 K, solid copper is always cold.

(d) Calculate the degeneracy pressure (Equation 5.46) of copper, in the electron gas model.

P=23EtotV=23ħ2kF510π2m=3π22/3ħ25mρ5/3

Short Answer

Expert verified

aEF=1.055×1034J.s6.58×10-16eV.s29.109×10-31kg3π28.49×1028/m32/3=7.04eV.bV=5.25×10-3×3×108=1.57×106m/scT=7.04eV8.62×10-5eV/K=8.17×104KdP=3π22/3ħ25mρ5/3=3π22/31.055×10-34259.109×10-318.49×10285/3N/m2=3.84×1010N/m2

Step by step solution

01

Given data

density of copper d =8.96gm/cm3

atomic weightof copper M =m=63.5gm/mol

02

(a) Calculating the Fermi energy for copper

EF=ħ2m3ρπ22/3.ρ=NqV=NV=atomsmole×molesgm×gmvolume=NAM.dM=atomicmass=63.5gm/mol,d=density=8.96gm/cm3.ρ=6.02×10238.96gm/cm363.5gm=8.49×1022/cm3=8.49×1028/m3EF=1.055×10-34J.s6.58×10-16eV.s29.109×10-31kg3π28.49×1028/m32/3=7.04eV.

03

Step3:(b) Corresponding electron velocity

7.04eV=120.511×106eV/c2v2v2c2=14.08.511×106=2.76×10-5vc=5.25×10-3

so it’s nonrelativistic.v=5.25×10-3×3×108=1.57×106m/s

04

Step4:(c) Temperature

T=7.04eV8.62×10-5eV/K=8.17×104K

05

Step5:(d) Calculating the Degeneracy of copper

P=3π22/3ħ25mρ5/3=3π22/31.055×10-34259.109×10-318.49×10285/3N/m2=3.84×1010N/m2

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Most popular questions from this chapter

Derive the Stefan-Boltzmann formula for the total energy density in blackbody radiation

EV=(π2kB415ħ3C3)T4=7.57×10-16Jm-3K-4T4

We can extend the theory of a free electron gas (Section 5.3.1) to the relativistic domain by replacing the classical kinetic energy, E=p2/2m,,with the relativistic formula, E=p2c2+m2c4-mc2. Momentum is related to the wave vector in the usual way: p=hk. In particular, in the extreme relativistic limit, Epc=hck.

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