Only a shell of energy width of order near the Fermi energy can change occupation: much lower states are blocked by the Pauli exclusion principle. The thermal-shell estimate of electronic heat capacity counts
To recover the rough coefficient requested in the paper, assign each of these active particles an excitation energy of order . Then
The differentiation matters: the active shell itself widens as temperature rises. This argument explains the small linear-in- electronic heat capacity; its shell width and average excitation energy are heuristic, so it does not establish a precise numerical prefactor.
A controlled calculation from the Fermi-Dirac distribution gives a nearby but different result. At fixed particle number, the Sommerfeld expansion yields
Thus is a rough estimate of the exact free-electron coefficient , not an exact consequence of the stated density of states. Both require .

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