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gptkbp:instanceOf
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gptkb:mathematical_concept
|
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gptkbp:appliesTo
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stationary black holes
|
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gptkbp:category
|
theorems in general relativity
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gptkbp:contrastsWith
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gptkb:hairy_black_holes
|
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gptkbp:describes
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black holes
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gptkbp:field
|
gptkb:general_relativity
physics
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|
https://www.w3.org/2000/01/rdf-schema#label
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no-hair theorem
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gptkbp:implies
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all other information about matter forming a black hole disappears behind the event horizon
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gptkbp:influenced
|
gptkb:black_hole_thermodynamics
gptkb:information_paradox
|
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gptkbp:parameter
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marina
angular momentum
electric charge
|
|
gptkbp:proposedBy
|
gptkb:Werner_Israel
gptkb:John_Archibald_Wheeler
gptkb:Stephen_Hawking
gptkb:Brandon_Carter
|
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gptkbp:relatedConcept
|
gptkb:Reissner–Nordström_black_hole
gptkb:Kerr_black_hole
gptkb:Schwarzschild_black_hole
event horizon
uniqueness theorem
|
|
gptkbp:state
|
black holes are characterized by only three externally observable classical parameters
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|
gptkbp:yearProposed
|
1970s
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gptkbp:bfsParent
|
gptkb:General_Theory_of_Relativity
|
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gptkbp:bfsLayer
|
4
|