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In physics, the Rayleigh-Jeans Law, first proposed in the early 20th century, attempts to describe the spectral radiance of electromagnetic radiation at all wavelengths from a black body at a given temperature. For wavelength λ, it is;

${\displaystyle f(\lambda )={\frac {2\pi ckT}{\lambda ^{4}}}}$

where T is the temperature in kelvins, and k is Boltzmann's constant.

The law is derived from classical physics arguments. Lord Rayleigh first obtained the fourth-power dependence on wavelength in 1900; a more complete derivation, which included the proportionality constant, was presented by Rayleigh and Sir James Jeans in 1905. It agrees with experimental measurements for long wavelengths. However it predicts an energy output that diverges towards infinity as wavelengths grow smaller. This was not supported by experiments and the failure has become known as the ultraviolet catastrophe.

In 1900 Max Planck had obtained a different law:

${\displaystyle f(\lambda )={\frac {2\pi c^{2}}{\lambda ^{5}}}~{\frac {h}{e^{\frac {hc}{\lambda kT}}-1}}}$

where h is Planck's constant and c is the speed of light. This is Planck's law of black body radiation expressed in terms of wavelength λ = c /ν. The Planck law does not suffer from an ultraviolet catastrophe, and agrees well with the experimental data, but its full significance was only appreciated several years later. In the limit of very high temperatures or long wavelengths, the term in the exponential becomes small, and so the denominator becomes approximately hc /λkT. This gives back the Rayleigh-Jeans Law.

See also

• John William Strutt, 3rd Baron Rayleigh
• Wien's displacement law
• Stefan-Boltzmann law

External links

• Rayleigh-Jeans Law and Schrodinger's Cat

• Foundational quantum physics