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gptkbp:instanceOf
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physical phenomenon
theoretical prediction
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gptkbp:basedOn
|
gptkb:general_relativity
gptkb:quantum_field_theory
thermodynamics
|
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gptkbp:category
|
gptkb:theoretical_physics
astrophysics
black hole physics
|
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gptkbp:cause
|
black hole evaporation
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gptkbp:causedBy
|
quantum effects near event horizon
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gptkbp:citation
|
gptkb:Nature_248,_30–31_(1974)
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gptkbp:describedBy
|
gptkb:Stephen_Hawking
|
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gptkbp:emissionType
|
thermal radiation
|
|
gptkbp:emits
|
black holes
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gptkbp:explains
|
black hole evaporation
|
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gptkbp:hasAnalogue
|
gptkb:Unruh_effect
gptkb:sonic_black_holes
laboratory analogues
|
|
gptkbp:hasModel
|
Hawking temperature formula
|
|
gptkbp:hasNotBeenObserved
|
directly
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Hawking radiation
|
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gptkbp:implies
|
black holes can eventually disappear
black holes can lose mass
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gptkbp:isQuantumEffect
|
true
|
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gptkbp:namedAfter
|
gptkb:Stephen_Hawking
|
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gptkbp:powerSource
|
gravitational energy of black hole
|
|
gptkbp:predicts
|
1974
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gptkbp:relatedTo
|
gptkb:cosmology
gptkb:quantum_gravity
gptkb:information_paradox
black holes
thermodynamics of black holes
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|
gptkbp:temperatureDependsOn
|
black hole mass
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gptkbp:temperatureIncreasesAs
|
black hole mass decreases
|
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gptkbp:bfsParent
|
gptkb:Stephen_Hawking
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gptkbp:bfsLayer
|
3
|