Summary

Max Planck Eight Lectures on Theoretical Physics… (1915)

Following the preparatory considerations of the last lecture we shall treat today the problem which we have come to recognize as one of the most important in the theory of heat radiation: the establishment of that universal function which governs the energy distribution in the normal spectrum. The means for the solution of this problem will be furnished us through the calculation of the entropy of a resonator placed in a vacuum filled with black radiation and thereby excited into stationary vibrations.
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Max Planck Eight Lectures on Theoretical Physics… (1915)

Accordingly, we have to consider the energy of a resonator placed in a stationary field of black radiation as a constant mean value of many disordered independent individual values, and this procedure agrees with the fact that every measurement of the intensity of heat radiation is extended over an enormous number of vibration periods. The entropy of a resonator is then to be calculated from the existing probability that the energy of the radiator possesses a definite mean value within a certain time interval.
Source: Wikisource

Max Planck Eight Lectures on Theoretical Physics… (1915)

In accordance with what we have seen in connection with the elucidation of the second law through atomistic ideas, the second law is only applicable to a physical system when we consider the quantities which determine the state of the system as mean values of numerous disordered individual values, and the probability of a state is then equal to the number of the numerous, a priori equally probable, complexions which make possible the realization of the state.
Source: Wikisource

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