light quanta

The equation explained

ϱ=αν3e−βνT\varrho = \alpha \nu^3 e^{-\beta \frac{\nu}{T}}
In wordsThe radiation's energy per unit volume and unit frequency equals the constant α times the frequency cubed, times e raised to minus the constant β times the frequency over the absolute temperature.OverviewWien's law for black radiation. The paper knows it is not exactly valid, but experiment had confirmed it very well where ν/T is large, and section 4 builds on it with its results limited to that region.Full explanationSection 4 bases its calculation on the law W. Wien originally set up for black radiation. The paper says plainly that observations show it is not exactly valid, but that for large values of ν/T\nu/T experiment had confirmed it very completely, so the results that follow hold only within certain limits: high frequency and low density. Compared with Planck's formula of section 2 it lacks the −1-1 in the denominator. Where βνT\frac{\beta \nu}{T} is large the exponential is huge and the −1-1 makes no difference, so there the two laws agree. The same constants α\alpha and β\beta appear in both.Every stepϱν=αν3eβνT−1\varrho_\nu = \frac{\alpha \nu^3}{e^{\frac{\beta \nu}{T}} - 1}Planck's formula, from section 2, for comparison.eβνT−1≈eβνTe^{\frac{\beta \nu}{T}} - 1 \approx e^{\frac{\beta \nu}{T}}Where βνT\frac{\beta \nu}{T} is large the exponential is very large, and taking one away changes it very little.ϱ=αν3eβνT=αν3e−βνT\varrho = \frac{\alpha \nu^3}{e^{\frac{\beta \nu}{T}}} = \alpha \nu^3 e^{-\beta \frac{\nu}{T}}Dividing by an exponential is multiplying by the exponential of minus its exponent: Wien's law as the paper prints it. The paper takes the law from Wien and from experiment; this comparison only shows where the two formulas agree.Also

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