Tolman-Oppenheimer-Volkoff limit
GPTKB entity
Statements (48)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:observatory
|
| gptkbp:allows |
mass of stable neutron stars
|
| gptkbp:applies_to |
gptkb:physicist
gptkb:spacecraft supernova explosions |
| gptkbp:borders |
neutron star stability
|
| gptkbp:consequences |
gptkb:Einstein's_field_equations
gravitational wave astronomy |
| gptkbp:defines |
the upper mass limit for neutron stars.
|
| gptkbp:developed_by |
theoretical models of neutron stars
|
| https://www.w3.org/2000/01/rdf-schema#label |
Tolman-Oppenheimer-Volkoff limit
|
| gptkbp:is_a_framework_for |
massive stars
|
| gptkbp:is_affected_by |
neutron star formation
|
| gptkbp:is_approximately |
2 to 3 solar masses
|
| gptkbp:is_associated_with |
neutron star mergers
|
| gptkbp:is_connected_to |
pulsar observations
|
| gptkbp:is_critical_for |
stellar astrophysics
|
| gptkbp:is_described_as |
the lifecycle of stars
maximum mass of a neutron star |
| gptkbp:is_discussed_in |
gptkb:literary_work
astrophysical models |
| gptkbp:is_essential_for |
understanding stellar evolution
compact objects in the universe |
| gptkbp:is_influenced_by |
theoretical astrophysics
equation of state of nuclear matter |
| gptkbp:is_related_to |
black hole formation
|
| gptkbp:is_studied_in |
high-energy physics
|
| gptkbp:is_tested_for |
observational data
|
| gptkbp:is_used_by |
neutron star properties
|
| gptkbp:is_used_in |
astrophysics
|
| gptkbp:key |
nuclear astrophysics
|
| gptkbp:measures |
gravitational collapse
|
| gptkbp:named_after |
gptkb:J._Anselm_Volkoff
gptkb:Leo_Tolman gptkb:J._Robert_Oppenheimer |
| gptkbp:related_concept |
modern astrophysics
|
| gptkbp:related_to |
gptkb:general_relativity
neutron degeneracy pressure |
| gptkbp:resulted_in |
quantum mechanics principles
|
| gptkbp:significance |
high-energy astrophysics
|
| gptkbp:subject |
research in theoretical physics
theoretical investigation |
| gptkbp:theory |
for neutron stars
neutron star characteristics |
| gptkbp:was_a_factor_in |
stellar collapse
stellar mass distribution |
| gptkbp:bfsParent |
gptkb:Richard_C._Tolman
|
| gptkbp:bfsLayer |
3
|