Penrose singularity theorem
E1018070
The Penrose singularity theorem is a fundamental result in general relativity showing that, under physically reasonable conditions such as gravitational collapse, spacetime must contain singularities where classical physics breaks down.
All labels observed (1)
| Label | Occurrences |
|---|---|
| Penrose singularity theorem canonical | 1 |
Statements (47)
| Predicate | Object |
|---|---|
| instanceOf |
result in mathematical physics
ⓘ
singularity theorem ⓘ theorem in general relativity ⓘ |
| appliesTo |
Lorentzian manifolds
NERFINISHED
ⓘ
spacetimes satisfying Einstein field equations ⓘ |
| assumes |
classical general relativity is valid
ⓘ
existence of a closed trapped surface ⓘ existence of a non-compact Cauchy surface or appropriate causality conditions ⓘ global hyperbolicity is violated by trapped surface formation ⓘ null energy condition ⓘ |
| author | Roger Penrose NERFINISHED ⓘ |
| concludes |
breakdown of classical spacetime description
ⓘ
existence of singularities in spacetime ⓘ spacetime is null geodesically incomplete ⓘ |
| countryOfOrigin | United Kingdom ⓘ |
| describedAs | first rigorous proof of generic singularity formation in gravitational collapse ⓘ |
| field |
differential geometry
ⓘ
general relativity NERFINISHED ⓘ gravitational physics ⓘ mathematical relativity ⓘ |
| implies |
black hole formation leads to geodesic incompleteness
ⓘ
singularities form in gravitational collapse under generic conditions ⓘ |
| influenced |
development of modern black hole theory
ⓘ
research on quantum gravity ⓘ study of global properties of spacetime ⓘ |
| language | English ⓘ |
| motivationFor | cosmic censorship hypothesis NERFINISHED ⓘ |
| namedAfter | Roger Penrose NERFINISHED ⓘ |
| originalTitle | Gravitational Collapse and Space-Time Singularities NERFINISHED ⓘ |
| publishedIn | Physical Review Letters NERFINISHED ⓘ |
| relatedTo |
Hawking singularity theorem
NERFINISHED
ⓘ
Hawking–Penrose singularity theorems NERFINISHED ⓘ black hole physics ⓘ cosmic censorship conjecture NERFINISHED ⓘ gravitational collapse ⓘ |
| requires |
Einstein field equations with reasonable matter content
ⓘ
smooth spacetime manifold ⓘ |
| status | widely accepted in classical general relativity ⓘ |
| topic |
causal structure
ⓘ
geodesic incompleteness ⓘ spacetime singularities ⓘ |
| usesConcept |
Raychaudhuri equation
NERFINISHED
ⓘ
causal structure of spacetime ⓘ global techniques in Lorentzian geometry ⓘ null geodesic congruence ⓘ trapped surface ⓘ |
| yearProved | 1965 ⓘ |
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.