phenomenon 49.19 Neutron stars reach two solar masses

open in the book · parts/05-general-relativity-cosmology/08-compact-stars.tex:1293 · p. 1355

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phenomenon 49.19: Neutron stars reach two solar masses49.19proposition 49.12: Buchdahl bound49.12theorem 49.9: Tolman–Oppenheimer–Volkoff equations49.9proof : ch:08-compact-stars@proof-14proofequation 49.21: eq:compact-uniform-pc49.21example 49.11: The uniform-density star49.11proof : ch:08-compact-stars@proof-9proofdefinition 44.16: Perfect fluid44.16equation 49.14: eq:compact-efe49.14equation 49.16: eq:compact-perfect-fluid49.16postulate 44.3: Einstein field equations44.3proof : ch:08-compact-stars@proof-8proof

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typedirectionnode provenancewhere
cites A Massive Pulsar in a Compact Relativistic Binary derived parts/05-general-relativity-cosmology/08-compact-stars.tex:1300
cites Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar derived parts/05-general-relativity-cosmology/08-compact-stars.tex:1301
cites A two-solar-mass neutron star measured using Shapiro delay derived parts/05-general-relativity-cosmology/08-compact-stars.tex:1299
cites Refined Mass and Geometric Measurements of the High-mass PSR J0740+6620 derived parts/05-general-relativity-cosmology/08-compact-stars.tex:1301
cites Maximum Mass of a Neutron Star derived parts/05-general-relativity-cosmology/08-compact-stars.tex:1307
depends_on Buchdahl bound declared parts/05-general-relativity-cosmology/08-compact-stars.tex:1310
depends_on Tolman–Oppenheimer–Volkoff equations declared parts/05-general-relativity-cosmology/08-compact-stars.tex:1310
proves ch:08-compact-stars@proof-14 declared parts/05-general-relativity-cosmology/08-compact-stars.tex:1313