Rayleigh–Jeans law at low frequencies
E31549
The Rayleigh–Jeans law at low frequencies is the classical approximation for blackbody radiation that accurately describes the long-wavelength, low-energy limit of Planck’s radiation spectrum.
Observed surface forms (1)
| Surface form | Occurrences |
|---|---|
| Rayleigh–Jeans law | 2 |
Statements (46)
| Predicate | Object |
|---|---|
| instanceOf |
approximation
ⓘ
classical limit of Planck’s law ⓘ physical law ⓘ |
| accuratelyDescribes | long-wavelength tail of blackbody spectrum ⓘ |
| appliesTo |
long wavelengths
ⓘ
low frequencies ⓘ low photon energies ⓘ |
| associatedWith | ultraviolet catastrophe when extrapolated to high frequencies ⓘ |
| assumes |
classical electromagnetic field
ⓘ
continuous energy spectrum ⓘ electromagnetic modes have energy kT per degree of freedom ⓘ |
| context | thermodynamic equilibrium of radiation in a cavity ⓘ |
| contrastWith | Wien’s law at high frequencies ⓘ |
| dependsOn |
absolute temperature T
ⓘ
frequency ν ⓘ wavelength λ ⓘ |
| derivedFrom |
classical statistical mechanics
ⓘ
equipartition theorem ⓘ |
| describes | spectral radiance of blackbody radiation ⓘ |
| domain | blackbody radiation ⓘ |
| failsAt |
high frequencies
ⓘ
short wavelengths ⓘ |
| field |
classical electrodynamics
ⓘ
statistical physics ⓘ thermal radiation ⓘ |
| formulaInFrequencyForm | B_ν(T) = (2ν²kT)∕c² ⓘ |
| formulaInWavelengthForm | B_λ(T) = (2ckT)∕λ⁴ ⓘ |
| historicalRole | motivated development of quantum theory ⓘ |
| implies | energy density of radiation grows without bound with frequency in classical theory ⓘ |
| isApproximationOf |
Planck radiation law
ⓘ
surface form:
Planck’s law of blackbody radiation
|
| isClassicalLimitOf |
Planck radiation law
ⓘ
surface form:
Planck’s radiation law
|
| isValidInLimit |
hν ≪ kT
ⓘ
λ ≫ hc∕kT ⓘ |
| namedAfter |
James Jeans
ⓘ
Lord Rayleigh ⓘ |
| predicts |
spectral radiance proportional to temperature T
ⓘ
spectral radiance proportional to λ⁻⁴ in wavelength domain ⓘ spectral radiance proportional to ν² in frequency domain ⓘ |
| relatesQuantity |
spectral radiance per unit frequency
ⓘ
spectral radiance per unit wavelength ⓘ |
| usedFor | approximating cosmic microwave background spectrum at low frequencies ⓘ |
| usedIn |
microwave regime analysis
ⓘ
radio astronomy ⓘ |
| usesConstant |
Boltzmann constant
ⓘ
surface form:
Boltzmann constant k
speed of light c ⓘ |
| validFor | hν∕kT ≪ 1 ⓘ |
Referenced by (3)
Full triples — surface form annotated when it differs from this entity's canonical label.
this entity surface form:
Rayleigh–Jeans law
this entity surface form:
Rayleigh–Jeans law