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nydus/The Theory of Heat RadiationPublic
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Page 117 of 235
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103.

A further example of the application of the two principles of thermodynamics is afforded by the irreversible expansion of originally black radiation of volume V and temperature T to the larger volume V as considered above in [sect:70.] Sec. 70, but in the absence of any absorbing or emitting substance whatever. Then not only the total energy but also the energy of every separate frequency ν remains constant; hence, when on account of diffuse reflection from the walls the radiation has again become uniform in all directions, 𝗎νV=𝗎νV; moreover by this relation, according to [eqn:(118)] (118), the temperature Tν' of the monochromatic radiation of frequency ν in the final state is determined. The actual calculation, however, can be performed only with the help of equation [eqn:(275)] (275) (see below). The total entropy of radiation, i.e., the sum of the entropies of the radiations of all frequencies, V0𝗌νdν, must, according to the second principle, be larger in the final state than in the original state. Since Tν has different values for the different frequencies ν, the final radiation is no longer black. Hence, on subsequent introduction of a carbon particle into the cavity, a finite change of the distribution of energy is obtained, and simultaneously the entropy increases further to the value S calculated in [eqn:(82)] (82).

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