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

§7 · fluorescence and its conditions

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 144

Stokes's rule

If each exciting quantum of frequency ν1\nu_1 is absorbed and on its own gives rise to a light quantum of frequency ν2\nu_2, the energy principle requires RNβν2≦RNβν1\frac{R}{N}\beta\nu_2 \leqq \frac{R}{N}\beta\nu_1, that is ν2≦ν1\nu_2 \leqq \nu_1, which is the known rule of Stokes.

As printed

Wenn die photolumineszierende Substanz nicht als eine beständige Quelle von Energie anzusehen ist, so kann nach dem Energieprinzip die Energie eines erzeugten Energiequants nicht größer sein als die eines erzeugenden Lichtquants; es muß also die Bezeichnung gelten: RNβν2≦RNβν1\frac{R}{N} \beta \nu_2 \leqq \frac{R}{N} \beta \nu_1Gas constantAvogadro's numberSpectral constant BFrequency of the emitted lightFrequency of the absorbed lightExplain this equation oder ν2≦ν1.\nu_2 \leqq \nu_1 .Frequency of the emitted lightFrequency of the absorbed lightExplain this equation Dies ist die bekannte Stokessche Regel.

Text on page 144 of the German source, § 7, paragraph 1

In modern notation

h ν2≤h ν1h\,\nu_2 \le h\,\nu_1

  • Premise: The photoluminescent substance is not to be regarded as a permanent source of energy; only then does the energy principle bound the produced quantum.
  • Premise: Each exciting quantum acts on its own, at least when the exciting quanta are sparse enough; the absorption may also produce quanta of other frequencies and energy of another kind, such as heat.
  • Conditional: The paper names when deviations are conceivable: when so many quanta are being transformed at once that one produced quantum can take its energy from several, and when the exciting or produced light is not of the kind Wien's law describes, for instance light from a body so hot that Wien's law fails at the wavelength in question.

Decoder

ν1\nu_1
The frequency of the exciting light, absorbed by the photoluminescent substance.
ν2\nu_2
The frequency of the light the substance produces.
RNβν\frac{R}{N}\beta\nu
The energy of one quantum of light of frequency ν\nu, taken from § 6 for both the exciting and the produced light.

Try it

Where this stops: The limit on frequency holds under these conditions; it does not forbid higher-frequency emission in general. The budget does not predict actual material rates or spectra. A dense field need not satisfy the independent-quantum assumptions used in the analogy. Read the argument

Argument
A consequence of the quantum picture and the energy principle
Model
Holds when each exciting quantum acts on its own and the substance supplies no energy
Evidence
Accounts for a rule already known from experiment
History
The rule was known before 1905, and the paper calls it known; its derivation from energy quanta is introduced here

§7 · fluorescence and its conditions

An energy budget has conditions

With one absorbed quantum, no extra energy, and a single emitted quantum, the outgoing energy cannot exceed the incoming energy. Extra thermal energy or multiple-quantum input changes those premises.