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.
At fixed volume and frequency, the entropy increase per added energy is 1/T. Inverting an admitted spectrum therefore determines an entropy derivative, but not yet its integration constant.
Let be energy per volume per frequency interval and 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.
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 and 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.
- Radiation of different frequencies can be separated without doing work and without supplying heat, so entropy and energy are sums over frequencies: and .
- 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 at each frequency.
- The energy must not change: . At a maximum, the entropy must not change to first order either: .
- Both statements must hold for every such change. That is possible only if with λ a number that does not depend on ν. So has the same value at every frequency.
- 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.
- Now warm black radiation of volume 1 by dT. Its entropy changes by . Because the derivative is the same at every frequency, it comes outside the integral, and what remains is the change of energy: .
- dE is the heat supplied, and the warming is reversible, so thermodynamics also gives .
- Compare the two expressions for dS. The common derivative is the inverse temperature, which in the explanatory letters is the formula below.
At fixed frequency, the partial derivative of spectral entropy density with respect to spectral energy density is inverse temperature.
- Read it in words: at fixed frequency, adding a little energy density raises the entropy density by that amount divided by the temperature.
- So a known radiation law, which gives T as a function of ρ at each ν, gives 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.
- 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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Read each operation, check its units and assumptions, or open the mathematical step behind it. These are modern teaching equations, not the equations as printed.
Explore the equation · Modern model notation
Entropy per unit of energy, at one frequency
grows with , at fixed , is one over .
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Each term and operation, in words
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Read the equation aloud in words
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.
At fixed volume and frequency, the entropy increase per added energy is 1/T. Inverting an admitted spectrum therefore determines an entropy derivative, but not yet its integration constant.
What this relies on
- Equilibrium thermodynamics holds, and energy and entropy add up over the spectrum.
- Vary the energy distribution at fixed volume and fixed total energy.
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