Eddington–Oppenheimer–Volkoff limit
GPTKB entity
AI-created image
Statements (19)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
astrophysical concept
|
| gptkbp:alsoKnownAs |
gptkb:Tolman–Oppenheimer–Volkoff_limit
|
| gptkbp:appliesTo |
gptkb:neutron_stars
|
| gptkbp:basisFor |
gptkb:Tolman–Oppenheimer–Volkoff_equation
|
| gptkbp:describes |
maximum mass of a neutron star
|
| gptkbp:exceedsLeadsTo |
black hole formation
|
| https://www.w3.org/2000/01/rdf-schema#label |
Eddington–Oppenheimer–Volkoff limit
|
| gptkbp:namedAfter |
gptkb:Arthur_Eddington
gptkb:George_Volkoff gptkb:J._Robert_Oppenheimer |
| gptkbp:publishedIn |
gptkb:Physical_Review
|
| gptkbp:relatedTo |
gptkb:Chandrasekhar_limit
gptkb:general_relativity gptkb:white_dwarfs |
| gptkbp:theorizedBy |
1939
|
| gptkbp:valuation |
approximately 2.1 solar masses
between 1.5 and 2.3 solar masses |
| gptkbp:bfsParent |
gptkb:Arthur_Eddington
|
| gptkbp:bfsLayer |
4
|