Ayón-Beato–García regular black hole solutions
E193999
The Ayón-Beato–García regular black hole solutions are theoretical, nonsingular black hole models in general relativity coupled to nonlinear electrodynamics that remove the central curvature singularity while preserving key black hole properties.
All labels observed (1)
| Label | Occurrences |
|---|---|
| Ayón-Beato–García regular black hole solutions canonical | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T1722283 — 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: Ayón-Beato–García regular black hole solutions Context triple: [Bardeen black hole model, relatedTo, Ayón-Beato–García regular black hole solutions]
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A.
Bardeen black hole model
The Bardeen black hole model is a theoretical proposal of a regular (non-singular) black hole solution in general relativity that avoids the central singularity by coupling gravity to nonlinear electrodynamics.
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B.
Kerr–Newman black hole
The Kerr–Newman black hole is a theoretical solution of Einstein’s field equations describing a rotating, electrically charged black hole characterized solely by its mass, angular momentum, and charge.
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C.
The Mathematical Theory of Black Holes
The Mathematical Theory of Black Holes is a landmark monograph that presents a rigorous, comprehensive treatment of the physics and mathematics underlying black hole solutions in general relativity.
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D.
Schwarzschild–Milne equations
The Schwarzschild–Milne equations are fundamental integro-differential equations in radiative transfer theory that describe the propagation and scattering of radiation through a plane-parallel, absorbing and emitting medium.
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E.
Schwarzschild black hole
A Schwarzschild black hole is the simplest theoretical black hole solution in general relativity, describing a static, spherically symmetric, non-rotating, uncharged mass with an event horizon defined by the Schwarzschild radius.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Target entity: Ayón-Beato–García regular black hole solutions Target entity description: The Ayón-Beato–García regular black hole solutions are theoretical, nonsingular black hole models in general relativity coupled to nonlinear electrodynamics that remove the central curvature singularity while preserving key black hole properties.
-
A.
Bardeen black hole model
The Bardeen black hole model is a theoretical proposal of a regular (non-singular) black hole solution in general relativity that avoids the central singularity by coupling gravity to nonlinear electrodynamics.
-
B.
Kerr–Newman black hole
The Kerr–Newman black hole is a theoretical solution of Einstein’s field equations describing a rotating, electrically charged black hole characterized solely by its mass, angular momentum, and charge.
-
C.
The Mathematical Theory of Black Holes
The Mathematical Theory of Black Holes is a landmark monograph that presents a rigorous, comprehensive treatment of the physics and mathematics underlying black hole solutions in general relativity.
-
D.
Schwarzschild–Milne equations
The Schwarzschild–Milne equations are fundamental integro-differential equations in radiative transfer theory that describe the propagation and scattering of radiation through a plane-parallel, absorbing and emitting medium.
-
E.
Schwarzschild black hole
A Schwarzschild black hole is the simplest theoretical black hole solution in general relativity, describing a static, spherically symmetric, non-rotating, uncharged mass with an event horizon defined by the Schwarzschild radius.
- F. None of above. chosen
Statements (47)
| Predicate | Object |
|---|---|
| instanceOf |
regular black hole solution
ⓘ
solution of Einstein equations ⓘ solution of Einstein–nonlinear electrodynamics system ⓘ theoretical model in general relativity ⓘ |
| aimsTo | provide singularity-free black hole model ⓘ |
| approaches | Reissner–Nordström solution at large radius ⓘ |
| avoids | central curvature singularity ⓘ |
| category |
exact solutions in general relativity
ⓘ
regular black hole models ⓘ |
| coreBehavior | de Sitter–like core near r = 0 ⓘ |
| coupledTo | nonlinear electrodynamics ⓘ |
| describedBy | specific nonlinear electrodynamics Lagrangian ⓘ |
| field |
general relativity
ⓘ
nonlinear electrodynamics ⓘ |
| framework | classical general relativity ⓘ |
| hasLimitCase | extremal regular black hole configuration ⓘ |
| hasParameter |
electric charge parameter
ⓘ
mass parameter ⓘ |
| hasProperty |
asymptotically flat
ⓘ
can possess inner Cauchy horizon ⓘ curvature-regular at r = 0 ⓘ electrically charged ⓘ event horizon may exist ⓘ nonsingular ⓘ regular black hole metric ⓘ spherically symmetric ⓘ static ⓘ |
| influenced | later constructions of regular black holes in modified gravity ⓘ |
| introducedBy |
Alberto García
ⓘ
Eloy Ayón-Beato ⓘ |
| metricType | Lorentzian metric ⓘ |
| motivatedBy |
removal of black hole singularities
ⓘ
search for regular black hole geometries ⓘ |
| preserves | key black hole properties ⓘ |
| publicationDecade | 1990s ⓘ |
| reducesTo | Reissner–Nordström black hole in weak-field limit ⓘ |
| relatedTo |
Bardeen black hole model
ⓘ
surface form:
Bardeen regular black hole
Hayward black hole model ⓘ
surface form:
Hayward regular black hole
|
| satisfies | Einstein field equations with nonlinear electromagnetic source ⓘ |
| spacetimeDimension | 4 ⓘ |
| usedIn |
analyses of Hawking radiation from regular black holes
ⓘ
gravitational lensing studies of regular black holes ⓘ quasinormal mode analyses of regular black holes ⓘ studies of black hole evaporation without singularities ⓘ studies of regular black hole thermodynamics ⓘ tests of cosmic censorship with regular metrics ⓘ |
| violates | standard energy conditions in some regions ⓘ |
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Subject: Ayón-Beato–García regular black hole solutions Description of subject: The Ayón-Beato–García regular black hole solutions are theoretical, nonsingular black hole models in general relativity coupled to nonlinear electrodynamics that remove the central curvature singularity while preserving key black hole properties.
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.