theorem 49.9 Tolman–Oppenheimer–Volkoff equations

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theorem 49.9: Tolman–Oppenheimer–Volkoff equations49.9definition 44.16: Perfect fluid44.16equation 49.14: eq:compact-efe49.14equation 49.16: eq:compact-perfect-fluid49.16postulate 44.3: Einstein field equations44.3example 49.11: The uniform-density star49.11phenomenon 49.19: Neutron stars reach two solar masses49.19proof : ch:08-compact-stars@proof-8proofdefinition 44.15: Dust44.15proposition 44.37: Energy conditions for the perfect fluid44.37proposition 44.20: Perfect-fluid equations of motion44.20definition 44.2: Einstein tensor44.2corollary 44.24: Conservation is an integrability condition44.24phenomenon 49.18: Orbital decay of a binary pulsar49.18phenomenon 46.1: phen:gravitational-waves46.1proposition 44.29: Linearized field equations44.29proposition 44.4: Trace-reversed form44.4theorem 48.5: The Friedmann equations48.5theorem 44.42: The constraint equations44.42equation 49.18: eq:compact-tov49.18proposition 49.12: Buchdahl bound49.12proof : ch:08-compact-stars@proof-14proof

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depends_on Perfect fluid declared parts/05-general-relativity-cosmology/08-compact-stars.tex:679
depends_on eq:compact-efe declared parts/05-general-relativity-cosmology/08-compact-stars.tex:679
depends_on eq:compact-perfect-fluid declared parts/05-general-relativity-cosmology/08-compact-stars.tex:679
depends_on Einstein field equations declared parts/05-general-relativity-cosmology/08-compact-stars.tex:679
depends_on The uniform-density star declared parts/05-general-relativity-cosmology/08-compact-stars.tex:804
depends_on Neutron stars reach two solar masses declared parts/05-general-relativity-cosmology/08-compact-stars.tex:1310
proves ch:08-compact-stars@proof-8 declared parts/05-general-relativity-cosmology/08-compact-stars.tex:683