Thermal Physics · Problem 18

Thermal Radiation and Planck Distribution — Charles Kittel & Herbert Kroemer

Physics — Statistical Mechanics · isentropic-expansion-of-photon-gas

Problem

Isentropic expansion of photon gas. Consider the gas of photons of the thermal equilibrium radiation in a cube of volume VV at temperature τ\tau. Let the cavity volume increase; the radiation pressure performs work during the expansion, and the temperature of the radiation will drop. From the result for the entropy we know that τV1/3\tau V^{1/3} is constant in such an expansion. (a) Assume that the temperature of the cosmic black-body radiation was decoupled from the temperature of the matter when both were at 3000 K. What was the radius of the universe at that time, compared to now? If the radius has increased linearly with time, at what fraction of the present age of the universe did the decoupling take place? (b) Show that the work done by the photons during the expansion is W=(π2/15ℏ3c3)Viτi3(τi−τf).W = (\pi^2/15\hbar^3 c^3)V_i \tau_i^3(\tau_i - \tau_f). The subscripts ii and ff refer to the initial and final states.

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