Pages 138, 139
The entropy of radiation and its temperature
Comparing two expressions for the entropy gained when black radiation of unit volume is warmed gives , which the paper calls the law of black radiation: from the entropy function one can find the radiation law, and from the radiation law, by integration, the function .
As printed
Durch Vergleich erhält man: Spectral entropy densitySpectral energy densityTemperature of the radiationExplain this equation Dies ist das Gesetz der schwarzen Strahlung. Man kann also aus der Funktion das Gesetz der schwarzen Strahlung und umgekehrt aus letzterem die Funktion durch Integration bestimmen mit Rücksicht darauf, daß für verschwindet.
Text on pages 138–139 of the German source, § 3, paragraph 4
In modern notation
- Premise: The warming is reversible and is the heat supplied; that is what allows .
- Premise: That does not depend on comes from the section's condition that the entropy be a maximum at fixed energy.
Decoder
- The entropy per unit volume and unit frequency of radiation whose energy density at the frequency is .
- The energy density per unit frequency, printed in §§ 3 and 4 without its subscript .
- vanishes for
- The condition that fixes the constant of integration when is found from the radiation law.
Try it
LQ-04: Take the derivative of the entropy density with respect to the energy density: does it come out as 1/T? Choose the preset “Derivative check: ds_nu/drho_nu against 1/T” there.
Where this stops: This is a thermodynamic comparison, not a microscopic account of every exchange. Integrating the derivative requires a boundary condition. Read the argument
- Argument
- A thermodynamic relation, used as a tool
- Model
- Exact for radiation in equilibrium
- Evidence
- A derivation, not evidence
- History
- Follows from thermodynamics available before 1905; the paper states it in this form