Metals — Question 6

Section 41-4 · Physics pages 6862–6863

Question 6 Pauli exclusion suppresses the electronic heat capacity For a degenerate free-electron gas use Ce = (π2/2)NkB(T/TF ), where TF = EF /kB. Take EF = 5.00 eV and kB = 8.617 × 10−5 eV/K. EF E thermal occupation window Schematic; labels, not drawing lengths, specify the data. (a) At 300 K find TF and the ratio to the classical value 3NkB/2. (b) Integrate the heat capacity from zero temperature to find the thermal energy increment and express it as a fraction of NEF .
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Question 6 - Solution Pauli exclusion suppresses the electronic heat capacity EF E thermal occupation window (a) Method and calculation TF = 5.00/(8.617 × 10−5) = 5.80 × 104 K . Ce 3NkB/2 = π2 3 300 TF = .0170 . (b) Interpretation and further calculation ∆U = ∫T 0 Ce(T′)dT′ = π2 4 NkBT 2 TF . ∆U/(NEF ) = π2 4 (T/TF )2 = 6.60 × 10−5 . Physical check Only states within an energy scale kBT of the Fermi surface can change occupation appreciably. The low-temperature expansion requires T much less than TF.

Question 6

Pauli exclusion suppresses the electronic heat capacity

For a degenerate free-electron gas use Ce=(π2/2)NkB(T/TF)C_e=(\pi^2/2)Nk_B(T/T_F), where TF=EF/kBT_F=E_F/k_B. Take EF=5.00eVE_F=5.00\,\mathrm{eV} and kB=8.617×10−5eV/Kk_B=8.617\times10^{-5}\,\mathrm{eV/K}.

Diagram shown in the original SVG worksheet.

  1. At 300 K find TFT_F and the ratio to the classical value 3NkB/23Nk_B/2.

  2. Integrate the heat capacity from zero temperature to find the thermal energy increment and express it as a fraction of NEFNE_F.

Question 6 - Solution

Pauli exclusion suppresses the electronic heat capacity

Diagram shown in the original SVG worksheet.

(a) Method and calculation

TF=5.00/(8.617×10−5)=5.80×104K.\boxed{T_F=5.00/(8.617\times10^{-5})=5.80\times10^4\,\mathrm K}.Ce3NkB/2=π23300TF=.0170.\boxed{\frac{C_e}{3Nk_B/2}=\frac{\pi^2}{3}\frac{300}{T_F}=.0170}.

(b) Interpretation and further calculation

ΔU=∫0TCe(T′)dT′=π24NkBT2TF.\Delta U=\int_0^TC_e(T\prime)dT\prime=\frac{\pi^2}{4}\frac{Nk_BT^2}{T_F}.ΔU/(NEF)=π24(T/TF)2=6.60×10−5.\boxed{\Delta U/(NE_F)=\frac{\pi^2}{4}(T/T_F)^2=6.60\times10^{-5}}.

Physical check

Only states within an energy scale kBT of the Fermi surface can change occupation appreciably. The low-temperature expansion requires T much less than TF.