Classical thermodynamics, heat transfer Thermal radiation Theorem
Planck's law
Builds on Black bodyThermal radiationThermodynamic temperatureEmissivity
Statement
Let a black body be in thermal equilibrium at absolute temperature . Let be the Planck constant, the speed of light in vacuum and the Boltzmann constant. Then, in every direction, its spectral radiance per unit frequency at frequency is Here spectral radiance is the emitted power per unit area normal to the direction, per unit solid angle and per unit frequency. Equivalently, the spectral radiance per unit wavelength at wavelength is
Remarks
Proof idea: in a cavity, the number of electromagnetic modes per unit volume and unit frequency is . If each mode of frequency can hold only energies with , the Boltzmann distribution gives the mean energy per mode. Multiplying gives the energy density , and the radiance is . The second form follows from with .
For the law reduces to the Rayleigh–Jeans law , and for to Wien's approximation . Integrating over frequency gives the Stefan–Boltzmann law, and locating the maximum gives Wien's displacement law. Max Planck found the law in 1900.
Going deeper
For a student
The law is the reference spectrum of radiative heat transfer: real surfaces are described by their emissivity relative to it. The two classical limits show where classical physics works: at low frequency equipartition is correct, and at high frequency the quantisation of energy suppresses emission. The same formula describes the cosmic microwave background, which fits a black-body spectrum at about K.
Reading path
To understand this page from the ground up, read these 5 pages in order. The foundations come first.
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- no evidence level
- Black body concept
- Emissivity concept
- Thermal radiation concept
- Thermodynamic temperature concept
- Planck's law statement
Where this leads
5 pages build on this one.
Further reading
About this page
| Tag | QKQ0V5S04R |
|---|---|
| URI | m2://QKQ0V5S04R |
| Kind | statement, theorem |
| Writing | W0 stub |
| MSC | 80A21, 78A40, 82B30 |
| Status | This copy of the site has no build data. Run m2 status QKQ0V5S04R. |
| About | Black body |
| Uses | Black body, Thermal radiation, Thermodynamic temperature, Emissivity |
| Same as | |
| Changed | 3 November 2026 |
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