Tolman– Oppenheimer– Volkoff limit
GPTKB entity
Statements (24)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:observatory
|
| gptkbp:applies_to |
gptkb:physicist
high-energy astrophysics |
| gptkbp:developed_by |
gptkb:Einstein's_field_equations
|
| https://www.w3.org/2000/01/rdf-schema#label |
Tolman– Oppenheimer– Volkoff limit
|
| gptkbp:is_analyzed_in |
stability of neutron stars
|
| gptkbp:is_approximately |
2 to 3 solar masses
|
| gptkbp:is_associated_with |
neutron star collapse
|
| gptkbp:is_critical_for |
stellar evolution
|
| gptkbp:is_described_as |
maximum mass of a neutron star
|
| gptkbp:is_discussed_in |
astrophysical literature
|
| gptkbp:is_influenced_by |
equation of state of nuclear matter
|
| gptkbp:is_related_to |
black hole formation
|
| gptkbp:is_used_for |
massive stars
|
| gptkbp:named_after |
gptkb:J._Robert_Oppenheimer
gptkb:George_Volkoff gptkb:Richard_Tolman |
| gptkbp:related_concept |
astrophysics
|
| gptkbp:related_to |
gptkb:general_relativity
neutron degeneracy pressure |
| gptkbp:significance |
gptkb:supernova_remnants
|
| gptkbp:theory |
compact stars
|
| gptkbp:bfsParent |
gptkb:Richard_C._Tolman
|
| gptkbp:bfsLayer |
3
|