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gptkbp:instanceOf
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exact solution in general relativity
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|
gptkbp:admission
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gptkb:Penrose_process
superradiance
frame dragging
closed timelike curves (inside ring singularity)
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gptkbp:coordinatesUsed
|
gptkb:Boyer–Lindquist_coordinates
|
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gptkbp:describes
|
rotating uncharged black hole
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gptkbp:discoveredBy
|
gptkb:Roy_Kerr
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gptkbp:discoveredIn
|
1963
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gptkbp:hasAngularMomentum
|
true
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|
gptkbp:hasErgosphere
|
true
|
|
gptkbp:hasEventHorizon
|
true
|
|
gptkbp:hasModel
|
rotating astrophysical black holes
|
|
gptkbp:hasNoElectricCharge
|
true
|
|
gptkbp:hasPetrovType
|
D
|
|
gptkbp:hasSingularity
|
ring singularity
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Kerr spacetime
|
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gptkbp:isAsymptoticallyFlat
|
true
|
|
gptkbp:isAxisymmetric
|
true
|
|
gptkbp:isMathematicallyDescribedBy
|
gptkb:Kerr_metric
|
|
gptkbp:isStationary
|
true
|
|
gptkbp:isVacuumSolution
|
true
|
|
gptkbp:measures
|
gptkb:Kerr_metric
|
|
gptkbp:parameter
|
marina
angular momentum
|
|
gptkbp:reduces
|
Schwarzschild spacetime (when spin is zero)
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gptkbp:relatedTo
|
gptkb:Schwarzschild_spacetime
gptkb:Kerr–Newman_spacetime
gptkb:Reissner–Nordström_spacetime
|
|
gptkbp:solvedBy
|
gptkb:Einstein_field_equations
|
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gptkbp:usedIn
|
astrophysics
black hole physics
gravitational wave research
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gptkbp:bfsParent
|
gptkb:Schwarzschild_spacetime
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gptkbp:bfsLayer
|
6
|