Pdf - Solved Problems In Thermodynamics And Statistical Physics

PV = nRT

where f(E) is the probability that a state with energy E is occupied, EF is the Fermi energy, k is the Boltzmann constant, and T is the temperature. PV = nRT where f(E) is the probability

f(E) = 1 / (e^(E-EF)/kT + 1)

PV = nRT

where f(E) is the probability that a state with energy E is occupied, EF is the Fermi energy, k is the Boltzmann constant, and T is the temperature.

f(E) = 1 / (e^(E-EF)/kT + 1)