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What is Fermi Distribution Function Explained about?

Here are the steps to solve the examples: (1) f(E) = 1/[exp((E-EF)/kT)+1] Put E-EF = 0.01 eV, T = 200K, k = 1.38x10-23 J/K f(E) = 1/[exp(0.01/1.38x10-23 x 200)+1] = 0.499986 (2) Let E-EF = kT. Then, f(E) = 1/[exp(1)+1] = 1/2 = 0.5 So at an energy kT above the Fermi energy, the Fermi function evaluates to 0.

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Random

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