definition 44.16 Perfect fluid

open in the book · parts/05-general-relativity-cosmology/03-einstein-field-equations.tex:729 · p. 1270

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definition 44.16: Perfect fluid44.16definition 44.15: Dust44.15proposition 44.37: Energy conditions for the perfect fluid44.37proposition 44.20: Perfect-fluid equations of motion44.20theorem 49.9: Tolman–Oppenheimer–Volkoff equations49.9definition 40.2: Four-velocity40.2phenomenon 40.6: Mass–energy equivalence40.6theorem 44.27: Newtonian correspondence of the field equations44.27definition 44.36: Energy conditions44.36proof : ch:03-einstein-field-equations@proof-19prooftheorem 44.19: Covariant conservation of stress–energy44.19corollary 44.21: Dust flows on geodesics44.21proof : ch:03-einstein-field-equations@proof-10proofequation 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-8proof

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typedirectionnode provenancewhere
depends_on Dust declared parts/05-general-relativity-cosmology/03-einstein-field-equations.tex:743
depends_on Energy conditions for the perfect fluid declared parts/05-general-relativity-cosmology/03-einstein-field-equations.tex:1521
depends_on Perfect-fluid equations of motion declared parts/05-general-relativity-cosmology/03-einstein-field-equations.tex:892
depends_on Tolman–Oppenheimer–Volkoff equations declared parts/05-general-relativity-cosmology/08-compact-stars.tex:679