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.
All labels observed (12)
How this entity was disambiguated
This entity first appeared as the object of triple T79864 — resolving that mention is where its identity was fixed. The disambiguator weighed these candidate entities and picked the highlighted one (or “None”, minting a new entity). This is how homonymy is resolved: the same surface form can point to different entities.
Target entity: Planck radiation law Context triple: [Bose–Einstein statistics, usedToExplain, Planck radiation law]
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A.
Einstein coefficients
Einstein coefficients are parameters in quantum theory that quantify the probabilities of absorption, spontaneous emission, and stimulated emission of radiation by atoms or molecules.
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B.
Bose–Einstein statistics
Bose–Einstein statistics is a quantum statistical framework that describes the distribution and collective behavior of indistinguishable bosons, underpinning phenomena such as Bose–Einstein condensation.
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C.
Huygens–Fresnel principle
The Huygens–Fresnel principle is a fundamental concept in wave optics that explains how every point on a wavefront acts as a source of secondary wavelets whose interference determines the wave’s subsequent propagation and diffraction.
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D.
Einstein field equations
The Einstein field equations are the core mathematical framework of general relativity, relating the curvature of spacetime to the distribution of matter and energy.
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E.
Does the Inertia of a Body Depend Upon Its Energy Content?
"Does the Inertia of a Body Depend Upon Its Energy Content?" is Albert Einstein’s 1905 paper that first articulated the mass–energy equivalence principle, commonly expressed as E = mc².
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Target entity: Planck radiation law Target entity description: 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.
-
A.
Einstein coefficients
Einstein coefficients are parameters in quantum theory that quantify the probabilities of absorption, spontaneous emission, and stimulated emission of radiation by atoms or molecules.
-
B.
Bose–Einstein statistics
Bose–Einstein statistics is a quantum statistical framework that describes the distribution and collective behavior of indistinguishable bosons, underpinning phenomena such as Bose–Einstein condensation.
-
C.
Huygens–Fresnel principle
The Huygens–Fresnel principle is a fundamental concept in wave optics that explains how every point on a wavefront acts as a source of secondary wavelets whose interference determines the wave’s subsequent propagation and diffraction.
-
D.
Einstein field equations
The Einstein field equations are the core mathematical framework of general relativity, relating the curvature of spacetime to the distribution of matter and energy.
-
E.
Does the Inertia of a Body Depend Upon Its Energy Content?
"Does the Inertia of a Body Depend Upon Its Energy Content?" is Albert Einstein’s 1905 paper that first articulated the mass–energy equivalence principle, commonly expressed as E = mc².
- F. None of above. chosen
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 radiation law self-linksurface differs ⓘ
surface form:
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 ⓘ |
How these facts were elicited
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Subject: Planck radiation law Description of subject: 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.
Referenced by (23)
Full triples — surface form annotated when it differs from this entity's canonical label.