Read · Light quanta: from entropy to an energy scale · Results

§4 · dilute radiation and the volume law

Einstein argues that light, when it is emitted or absorbed, behaves as if its energy came in separate quanta, and calls the idea a heuristic point of view. Follow all nine sections, from the trouble with classical radiation to the photoelectric effect.

The paper's results

Page 139

How the entropy of monochromatic radiation depends on its volume

Taking as its basis Wien's law, which experiment confirms for large ν/T\nu/T, the paper finds that the entropy of radiation of energy EE between ν\nu and ν+dν\nu + d\nu depends on the volume it occupies as S−S0=Eβνlg⁡(vv0)S - S_0 = \frac{E}{\beta\nu}\lg\left(\frac{v}{v_0}\right), a result valid only within certain limits.

As printed

Dasselbe wurde aber für große Werte von ν/T\nu/T sehr vollkommen durch das Experiment bestätigt. Wir legen diese Formel unseren Rechnungen zugrunde, behalten aber im Sinne, daß unsere Resultate nur innerhalb gewisser Grenzen gelten.

Beschränken wir uns darauf, die Abhängigkeit der Entropie von dem von der Strahlung eingenommenen Volumen zu untersuchen, und bezeichnen wir die Entropie der Strahlung mit S0S_0, falls dieselbe das Volumen v0v_0 besitzt, so erhalten wir: 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

Text on page 139 of the German source, § 4, paragraph 1 · Text on page 139 of the German source, § 4, paragraph 2

In modern notation

uν=A ν3 exp⁡(−B νT)u_\nu = A\,\nu^{3}\,\exp\left(-\frac{B\,\nu}{T}\right)
sν=−uνB ν (ln⁡(uνA ν3)−1)+C(ν)s_\nu = -\frac{u_\nu}{B\,\nu}\,\left(\ln\left(\frac{u_\nu}{A\,\nu^{3}}\right) - 1\right) + C\left(\nu\right)
S(V)−S(V0)=EB ν ln⁡(VV0)S\left(V\right) - S\left(V_{0}\right) = \frac{E}{B\,\nu}\,\ln\left(\frac{V}{V_{0}}\right)

  • Premise: The calculation rests on Wien's law, which the paper says is not exactly valid; its results hold only within certain limits, where Wien's law is confirmed, for large ν/T\nu/T.
  • Premise: The energy and the frequency band are held fixed; only the volume changes.

Decoder

EE
The energy of radiation whose frequency lies between ν\nu and ν+dν\nu + d\nu.
vv, v0v_0, S0S_0
The volume the radiation occupies, a reference volume, and the radiation's entropy when it occupies v0v_0.
β\beta
The constant of Wien's law, ϱ=αν3e−βν/T\varrho = \alpha\nu^3 e^{-\beta\nu/T}.
lg⁡\lg
The natural logarithm, as the paper prints it.

Try it

Where this stops: A moving mirror generally changes frequency and energy, so it is not this held-fixed comparison. The result is not valid merely because one of the two endpoint states is dilute. Read the argument

Where this stops: A positive inferred temperature alone is not a guarantee that the Wien approximation is accurate. The spectral constants are not initially interpreted as particle energies. Read the argument

Argument
A derivation from Wien's law
Model
Within the range of validity of Wien's law
Evidence
A derivation, not evidence
History
Introduced in this paper

§4 · dilute radiation and the volume law

The constant cannot simply be dropped

Inverting Wien’s law and integrating gives the entropy density plus a frequency-dependent constant. Requiring zero entropy density at zero radiation fixes that constant; it does not cancel automatically.

Compare two states, not a compression movie

For the same energy and narrow frequency band, Wien radiation gains entropy logarithmically with accessible volume. Both endpoint states must remain in the admitted regime.