A filled Fermi sphere has total kinetic energy (the check-yourself result of Section 8.5)

PHYSICS · Subjective · Fermi University Physics · Thermal, Statistical & Complex Systems · Condensed Matter, Materials & Soft Matter · Free electrons, energy bands and electronic structure

Condensed Matter Physics, Ch The free-electron gas: what Drude gets right and what only Fermi fixes

Problem

A filled Fermi sphere has total kinetic energy U=35NEFU=\tfrac35NE_F (the check-yourself result of Section 8.5), with EF=(ℏ2/2m)(3π2N/V)2/3E_F=(\hbar^2/2m)(3\pi^2N/V)^{2/3} depending on the volume VV through N/V=nN/V=n. The gas exerts an outward pressure P=−(∂U/∂V)NP=-(\partial U/\partial V)_N, exactly as a classical gas does. (a) Differentiate to show that P=25nEFP=\tfrac25nE_F. (b) Evaluate this degeneracy pressure for copper, using n=8.47×1028 m−3n=8.47\times10^{28}\,\mathrm{m^{-3}} and EF=7.03 eVE_F=7.03\,\mathrm{eV}, in gigapascals. (c) Differentiate once more to find the gas's own bulk modulus, B=−V dP/dVB=-V\,\mathrm{d}P/\mathrm{d}V, in terms of nn and EFE_F, evaluate it for copper and compare it with copper's measured bulk modulus of 140 GPa140\,\mathrm{GPa} (Chapter 7). Separately, what must balance the outward pressure PP for copper to sit in equilibrium with no pressure applied from outside?

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