Statistical Mechanics · Problem 3.15

The Grand Canonical Ensemble — R. K. Pathria

Physics — Statistical Mechanics · extreme-relativistic-gas

Problem

Show that the partition function QN(V,T)Q_N(V, T) of an extreme relativistic gas consisting of NN monatomic molecules with energy--momentum relationship ε=pc\varepsilon = pc, cc being the speed of light, is given by QN(V,T)=1N!{8πV(kThc)3}NQ_N(V,T) = \frac{1}{N!}\left\{8\pi V\left(\frac{kT}{hc}\right)^3\right\}^N Study the thermodynamics of this system, checking in particular that PV=13U,U/N=3kTandγ=43.PV = \tfrac{1}{3}U, \quad U/N = 3kT \quad \text{and} \quad \gamma = \tfrac{4}{3}. Next, using the inversion formula (3.4.7), derive an expression for the density of states g(E)g(E) of this system.

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