Tolman–Oppenheimer–Volkoff equation
GPTKB entity

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Statements (24)
Predicate | Object |
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gptkbp:instanceOf |
gptkb:algebra
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gptkbp:appliesTo |
non-rotating stars
spherically symmetric bodies |
gptkbp:describes |
hydrostatic equilibrium in relativistic stars
structure of neutron stars |
gptkbp:field |
gptkb:general_relativity
astrophysics |
gptkbp:form |
dP/dr = -G [ε(r) + P(r)/c^2][m(r) + 4πr^3P(r)/c^2]/[r(r-2Gm(r)/c^2)]
|
gptkbp:generalizes |
hydrostatic equilibrium equation
|
https://www.w3.org/2000/01/rdf-schema#label |
Tolman–Oppenheimer–Volkoff equation
|
gptkbp:namedAfter |
gptkb:George_Volkoff
gptkb:J._Robert_Oppenheimer gptkb:Richard_C._Tolman |
gptkbp:publicationYear |
1939
|
gptkbp:publishedIn |
gptkb:Physical_Review
|
gptkbp:relatedTo |
gptkb:Tolman–Oppenheimer–Volkoff_limit
energy density mass distribution pressure radius |
gptkbp:usedFor |
modeling neutron stars
studying compact objects |
gptkbp:bfsParent |
gptkb:Tolman–Oppenheimer–Volkoff_limit
|
gptkbp:bfsLayer |
4
|