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gptkbp:instanceOf
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gptkb:exact_solution_in_general_relativity
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gptkbp:coordinates
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gptkb:Boyer–Lindquist_coordinates
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gptkbp:describes
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gptkb:rotating_black_hole
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gptkbp:generalizes
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gptkb:Kerr–Newman_solution
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gptkbp:hasCausalStructure
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contains closed timelike curves inside inner horizon
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gptkbp:hasErgosphere
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yes
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gptkbp:hasEventHorizon
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yes
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gptkbp:hasNoElectricCharge
|
in original form
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gptkbp:hasSingularity
|
ring singularity
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gptkbp:isMathematicalModelOf
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rotating uncharged black hole
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gptkbp:isVacuumSolution
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yes
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gptkbp:measures
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asymptotically flat
axisymmetric
stationary
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gptkbp:parameter
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gptkb:marina
angular momentum
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gptkbp:proposedBy
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gptkb:Roy_Kerr
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gptkbp:reduces
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gptkb:Schwarzschild_solution
when angular momentum is zero
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gptkbp:satisfies
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gptkb:Einstein_field_equations
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gptkbp:solvedBy
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gptkb:general_relativity
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gptkbp:symmetry
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axial symmetry
time translation symmetry
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gptkbp:usedIn
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astrophysics
gravitational wave research
study of black holes
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gptkbp:yearProposed
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1963
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gptkbp:bfsParent
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gptkb:general_relativity
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gptkbp:bfsLayer
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4
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https://www.w3.org/2000/01/rdf-schema#label
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Kerr solution
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