Planck radiation law
E4994
Planck radiation law is a fundamental formula in quantum physics that describes the spectral distribution of electromagnetic radiation emitted by a black body in thermal equilibrium.
Aliases (9)
Statements (49)
| Predicate | Object |
|---|---|
| instanceOf |
law of black-body radiation
→
law of quantum physics → physical law → |
| appliesTo |
ideal black body
→
|
| assumes |
bosonic statistics for photons
→
electromagnetic modes in a cavity → thermal equilibrium → |
| dependsOnConstant |
Boltzmann constant
→
Planck constant → speed of light in vacuum → |
| derivedUsing |
Bose–Einstein statistics for photons
→
Planck distribution → |
| describes |
black-body radiation
→
spectral distribution of electromagnetic radiation → |
| domain |
thermal radiation
→
|
| expresses |
spectral radiance as function of frequency and temperature
→
spectral radiance as function of wavelength and temperature → |
| field |
electromagnetism
→
quantum physics → statistical mechanics → thermodynamics → |
| historicalSignificance |
marked birth of quantum theory
→
|
| implies |
energy quantization of electromagnetic modes
→
|
| introducedBy |
Max Planck
→
|
| involvesConcept |
black-body spectrum
→
quantization of energy levels → |
| involvesQuantity |
photon energy
→
photon occupation number → spectral radiance → |
| mathematicalForm |
spectral radiance proportional to 1/λ^5 divided by (exp(hc/(λkT)) − 1)
→
spectral radiance proportional to ν^3 divided by (exp(hν/kT) − 1) → |
| predicts |
peak wavelength of black-body spectrum depends on temperature
→
total emitted power increases with temperature → |
| reducesTo |
Rayleigh–Jeans law at low frequencies
→
Wien approximation at high frequencies → |
| relatedTo |
Stefan–Boltzmann law
→
Wien displacement law → |
| resolves |
ultraviolet catastrophe of classical physics
→
|
| usedIn |
astrophysics
→
cosmology → infrared thermography → radiative heat transfer calculations → remote sensing → thermal radiation modeling → |
| validFor |
macroscopic bodies approximating black bodies
→
|
| variable |
absolute temperature
→
frequency → wavelength → |
| yearProposed |
1900
→
|