Oppenheimer–Snyder model

E376

cosmological collapse solution gravitational collapse model solution in general relativity theoretical model

The Oppenheimer–Snyder model is a pioneering theoretical description of gravitational collapse in general relativity, providing one of the first rigorous treatments of how a massive star can form a black hole.

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All labels observed (4)

Label	Occurrences
On Continued Gravitational Contraction	1
Oppenheimer–Snyder model canonical	1
Oppenheimer–Snyder model of gravitational collapse	1
Oppenheimer–Snyder solution in general relativity	1

Statements (47)

Predicate	Object
instanceOf	cosmological collapse solution ⓘ gravitational collapse model ⓘ solution in general relativity ⓘ theoretical model ⓘ
assumes	dust equation of state ⓘ homogeneous matter distribution ⓘ no charge ⓘ no rotation ⓘ pressureless matter ⓘ spherical symmetry ⓘ
describes	collapse of a massive star ⓘ collapse of a pressureless dust sphere ⓘ formation of a black hole ⓘ gravitational collapse ⓘ
field	astrophysics ⓘ general relativity ⓘ relativistic astrophysics ⓘ
influenced	later work on realistic stellar collapse models ⓘ
introducedBy	Hartland Snyder ⓘ J. Robert Oppenheimer ⓘ
involves	Schwarzschild coordinates for the exterior ⓘ comoving coordinates for the interior ⓘ matching conditions at the stellar surface ⓘ
isConsidered	one of the first rigorous treatments of black hole formation ⓘ pioneering description of gravitational collapse ⓘ
isExampleOf	exact solution of Einstein field equations ⓘ idealized collapse model ⓘ
language	English ⓘ
matches	interior FLRW solution to exterior Schwarzschild solution ⓘ
neglects	pressure forces ⓘ radiation emission ⓘ rotation of the collapsing star ⓘ
paperTitle	Oppenheimer–Snyder model self-linksurface differs ⓘ surface form: On Continued Gravitational Contraction
predicts	finite proper time to collapse for comoving observers ⓘ formation of a singularity ⓘ formation of an event horizon ⓘ gravitational time dilation for distant observers ⓘ
publishedInJournal	Physical Review ⓘ
publishedInYear	1939 ⓘ
relatedTo	FLRW cosmological models ⓘ Penrose diagrams of gravitational collapse ⓘ Schwarzschild black hole ⓘ
usedFor	illustrating causal structure of collapse ⓘ pedagogical studies of black hole formation ⓘ testing numerical relativity codes ⓘ
usesMetric	FLRW cosmological models ⓘ surface form: Friedmann–Lemaître–Robertson–Walker metric Schwarzschild black hole ⓘ surface form: Schwarzschild metric

Referenced by (4)

Full triples — surface form annotated when it differs from this entity's canonical label.

J. Robert Oppenheimer → notableWork → Oppenheimer–Snyder model ⓘ

Oppenheimer–Snyder model → paperTitle → Oppenheimer–Snyder model self-linksurface differs ⓘ

this entity surface form: On Continued Gravitational Contraction

Hartland Snyder → notableWork → Oppenheimer–Snyder model ⓘ

this entity surface form: Oppenheimer–Snyder model of gravitational collapse

Hartland Snyder → notableFor → Oppenheimer–Snyder model ⓘ

this entity surface form: Oppenheimer–Snyder solution in general relativity