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.


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

Referenced by (16)
Subject (surface form when different) Predicate
Einstein coefficients
On a Heuristic Point of View Concerning the Production and Transformation of Light ("Planck’s black-body radiation law")
Stefan–Boltzmann law ("Planck’s law")
Wien displacement law
relatedTo
Max Planck ("black-body radiation law")
Max Planck ("Planck's law of black-body radiation")
knownFor
Boltzmann constant ("Planck blackbody radiation law")
appearsIn
Planck constant
appearsInEquation
Wien displacement law
approximationOf
Stefan–Boltzmann law ("Planck’s law of black-body radiation")
derivedFrom
Planck radiation law ("Planck distribution")
derivedUsing
Rayleigh–Jeans law at low frequencies ("Planck’s law of blackbody radiation")
isApproximationOf
Rayleigh–Jeans law at low frequencies ("Planck’s radiation law")
isClassicalLimitOf
k_B ("Planck distribution")
playsRoleIn
Kirchhoff's law of thermal radiation ("Planck's law of black-body radiation")
usedInDerivationOf
Bose–Einstein statistics
usedToExplain

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