Read · Light quanta: from entropy to an energy scale

§3 · temperature and entropy

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§3 · temperature and entropy

A derivation

A spectrum can determine an entropy derivative

How does equilibrium temperature constrain radiation entropy?

The 6 printed paragraphs this passage explains
  • §2, paragraph 4: From here on, black radiation is treated from experience, without any picture of how radiation is produced or travels.
  • §3, paragraph 1: The next argument is Wien's, from a well-known paper, and is included only for completeness.
  • §3, paragraph 2: Radiation filling a volume v is taken to be fully described by its energy density at every frequency. Since radiation of different frequencies can be separated without work or heat, its entropy is the volume times a sum over frequencies of an entropy density that depends on the density and the frequency.
  • §3, footnote 1: The footnote calls that assumption arbitrary: it is the simplest one, to be kept until experiment forces it to be dropped.
  • §3, paragraph 3: For black radiation the entropy is as large as it can be for the given energy, which means the rate at which the entropy density grows with the energy density is the same at every frequency.
  • §3, paragraph 4: Warming black radiation in a unit volume, and comparing with the rule that entropy grows by the added heat divided by the temperature, shows that this common rate is one over the temperature. That is the law of black radiation, so the entropy density can be found from the radiation law, and the radiation law from it.

Let ρν\rho_\nu be energy per volume per frequency interval and sνs_\nu the corresponding entropy density. At fixed volume, equilibrium maximizes entropy while keeping total energy fixed. Moving a small amount of energy from one spectral interval to another must give no first-order entropy gain at equilibrium.

Consequently the derivatives of entropy with respect to spectral energy density have the same value across the equilibrium spectrum. The thermodynamic identity dS/dE = 1/T, with other constraints fixed, identifies that common value.

(∂sν∂uν)ν=1T\left(\frac{\partial s_\nu}{\partial u_\nu}\right)_{\nu} = \frac{1}{T}

At fixed frequency, the partial derivative of spectral entropy density with respect to spectral energy density is inverse temperature.

Einstein attributes this thermodynamic reasoning to Wien. The next step is to express 1/T as a function of density by using Wien’s spectral law, not by assuming particles of light in advance.

Show every step here: A spectrum can determine an entropy derivative

Letters: the paper puts the radiation in a volume v, writes ρ for its density at each frequency ν, and writes φ(ρ, ν) for its entropy per unit volume and unit frequency. This explanation writes ρν\rho_\nu and sνs_\nu for the same two quantities. The paper takes it as given that the observable properties of the radiation are fixed once ρ is known for all frequencies; a footnote calls this assumption arbitrary, to be kept until experiment forces it to be dropped.

  1. Radiation of different frequencies can be separated without doing work and without supplying heat, so entropy and energy are sums over frequencies: S=v∫0∞φ(ρ,ν) dνS=v\int_0^\infty\varphi(\rho,\nu)\,d\nu and E=v∫0∞ρ dνE=v\int_0^\infty\rho\,d\nu.
  2. Black radiation is the equilibrium state: for the given energy, its entropy is as large as it can be. Take v = 1 and change the spectrum by a small amount δρδρ at each frequency.
  3. The energy must not change: ∫0∞δρ dν=0\int_0^\infty δρ\,d\nu=0. At a maximum, the entropy must not change to first order either: ∫0∞∂φ∂ρδρ dν=0\int_0^\infty\frac{\partial\varphi}{\partial\rho}δρ\,d\nu=0.
  4. Both statements must hold for every such change. That is possible only if ∫0∞(∂φ∂ρ−λ)δρ dν=0\int_0^\infty\left(\frac{\partial\varphi}{\partial\rho}-\lambda\right)δρ\,d\nu=0 with λ a number that does not depend on ν. So ∂φ/∂ρ\partial\varphi/\partial\rho has the same value at every frequency.
  5. A two-band check of that step: move a small amount of energy q out of band 1 and into band 2, keeping the total fixed. The entropy changes by q times (the derivative in band 2 minus the derivative in band 1). If the two derivatives differed, choosing the sign of q would raise the entropy, so at the maximum they are equal.
  6. Now warm black radiation of volume 1 by dT. Its entropy changes by dS=∫0∞∂φ∂ρdρ dνdS=\int_0^\infty\frac{\partial\varphi}{\partial\rho}d\rho\,d\nu. Because the derivative is the same at every frequency, it comes outside the integral, and what remains is the change of energy: dS=∂φ∂ρdEdS=\frac{\partial\varphi}{\partial\rho}dE.
  7. dE is the heat supplied, and the warming is reversible, so thermodynamics also gives dS=1TdEdS=\frac{1}{T}dE.
  8. Compare the two expressions for dS. The common derivative is the inverse temperature, which in the explanatory letters is the formula below.
(∂sν∂uν)ν=1T\left(\frac{\partial s_\nu}{\partial u_\nu}\right)_{\nu} = \frac{1}{T}

At fixed frequency, the partial derivative of spectral entropy density with respect to spectral energy density is inverse temperature.

  1. Read it in words: at fixed frequency, adding a little energy density raises the entropy density by that amount divided by the temperature.
  2. So a known radiation law, which gives T as a function of ρ at each ν, gives ∂φ/∂ρ\partial\varphi/\partial\rho as a function of ρ. Integrating recovers φ, once one more condition fixes the constant of integration: the paper requires φ to vanish when ρ = 0.
  3. The paper credits this reasoning to a celebrated work of W. Wien and includes it for completeness. It uses no picture of how radiation is produced or how it travels.
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Entropy per unit of energy, at one frequency

(∂sν∂uν)ν=1T\left(\frac{\partial s_\nu}{\partial u_\nu}\right)_{\nu} = \frac{1}{T}

grows with , at fixed , is one over .

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At fixed frequency, the partial derivative of the spectral entropy density with respect to the spectral energy density is one over the temperature.

At equilibrium, moving a little energy from one frequency interval to another gains no entropy to first order, so this derivative has one common value across the spectrum. The thermodynamic identity dS/dE = 1/T names that value.

Model assumptions and every term’s meaning
  • Radiation in equilibrium at fixed volume.
  • Entropy density and energy density are compared at one frequency.
  • These are modern teaching equations in SI notation, not a transcription of the printed paper. The paper writes phi for the entropy density.
Rate of change at fixed frequency
How much the entropy density rises per unit of added energy density, with the frequency held where it is. Read the prerequisite
One over the temperature
Thermodynamics defines temperature this way: dS/dE = 1/T, with the other constraints fixed. Read the prerequisite
What it asserts
At equilibrium every frequency interval gains the same entropy per unit of energy, and that common value is 1/T. Read the prerequisite
Spectral energy density
Radiation energy per cubic metre per unit of frequency. Read the prerequisite
Spectral entropy density
Entropy per cubic metre per unit of frequency; the paper writes it phi. Read the prerequisite
Frequency, held fixed
The comparison is made at one frequency; only the energy density changes. Read the prerequisite
Temperature
The temperature of the radiation in equilibrium. Read the prerequisite

Every term’s units were checked when this page was built. That checks the units, not the model. This equation is written for this edition in modern notation, not transcribed from the paper.

Modern qualifications

The variational calculation assumes that the radiation entropy can be represented by a function of spectral density and frequency. That is a stated thermodynamic assumption, not a derivation of a microscopic state-counting model.

Assumptions and limits: A spectrum can determine an entropy derivative

Assumed here

  • Equilibrium thermodynamics holds, and energy and entropy add up over the spectrum.
  • Vary the energy distribution at fixed volume and fixed total energy.

What this does not establish

  • This is a thermodynamic comparison, not a microscopic account of every exchange.
  • Integrating the derivative requires a boundary condition.

Source context: German source · English · Interlinear gloss · Facsimile

References

A. Einstein, Über einen die Erzeugung und Verwandlung des Lichtes betreffenden heuristischen Gesichtspunkt. Annalen der Physik (4), 17, 132–148 (1905).

A. Einstein, On the motion of particles suspended in liquids at rest required by the molecular-kinetic theory of heat. Annalen der Physik (4), 17, 549–560 (1905), §§1–5. Bibliographic pointer; this preview is not a source transcription or translation.

A. Einstein, Zur Elektrodynamik bewegter Körper. Annalen der Physik (4), 17, 891–921 (1905).

A. Einstein, Does the inertia of a body depend upon its energy content? Annalen der Physik (4), 18, 639–641 (1905). External 1923 Perrett–Jeffery translation, electronically transcribed by John Walker; its notation was modernized. A reference for this explanatory preview, not this edition’s translation or its pinned facsimile.

R. A. Millikan, A Direct Photoelectric Determination of Planck's "h". Physical Review (2), 7 (3), 355–388 (1916).

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