Translation

On a Heuristic Point of View Concerning the Generation and Transformation of Light

Über einen die Erzeugung und Verwandlung des Lichtes betreffenden heuristischen Gesichtspunkt

by A. Einstein

§ 4. Limiting law for the entropy of monochromatic radiation at low radiation density.

It does follow, to be sure, from the observations of “black radiation” so far that the law originally set up by Mr. W. Wien for “black radiation” ϱ=αν3e−βνT\varrho = \alpha \nu^3 e^{-\beta \frac{\nu}{T}}Spectral energy densitySpectral constant AFrequency of the lightSpectral constant BTemperature of the radiationExplain this equation is not exactly valid. But for large values of ν/T\nu/T it has been confirmed very completely by experiment. We take this formula as the basis of our calculations, but bear in mind that our results hold only within certain limits.

From this formula there follows first: 1T=−1βνlg⁡ϱαν3\frac{1}{T} = -\frac{1}{\beta \nu} \lg \frac{\varrho}{\alpha \nu^3}Temperature of the radiationSpectral constant BFrequency of the lightSpectral energy densitySpectral constant AExplain this equation and further, using the relation found in the preceding section: φ(ϱ,ν)=−ϱβν{lg⁡ϱαν3−1}.\varphi(\varrho, \nu) = -\frac{\varrho}{\beta \nu} \left\{ \lg \frac{\varrho}{\alpha \nu^3} - 1 \right\}.Spectral entropy densitySpectral energy densityFrequency of the lightSpectral constant BSpectral constant AExplain this equation Now let there be given a radiation of energy EE whose frequency lies between ν\nu and ν+dν\nu + d \nu. Let the radiation occupy the volume vv. The entropy of this radiation is: S=vφ(ϱ,ν)dν=−Eβν{lg⁡Evαν3dν−1}.S = v \varphi(\varrho, \nu) d \nu = -\frac{E}{\beta \nu} \left\{ \lg \frac{E}{v \alpha \nu^3 d \nu} - 1 \right\}.Radiation entropyVolumeSpectral entropy densitySpectral energy densityFrequency of the lightRadiation energy in the bandSpectral constant BSpectral constant AExplain this equation If we confine ourselves to investigating the dependence of the entropy on the volume occupied by the radiation, and denote by S0S_0 the entropy of the radiation when it has the volume v0v_0, we obtain: S−S0=Eβνlg⁡(vv0).S - S_0 = \frac{E}{\beta \nu} \lg \left( \frac{v}{v_0} \right).Radiation entropyRadiation entropyRadiation energy in the bandSpectral constant BFrequency of the lightVolumeVolumeExplain this equation

This equation shows that the entropy of a monochromatic radiation of sufficiently small density varies with the volume according to the same law as the entropy of an ideal gas or that of a dilute solution. The equation just found will be interpreted in what follows on the basis of the principle introduced into physics by Mr. Boltzmann, according to which the entropy of a system is a function of the probability of its state.

Bern, 17 March 1905.

(Received 18 March 1905.)