phenomenon 49.6 A maximum mass for a cold degenerate star

open in the book · parts/05-general-relativity-cosmology/08-compact-stars.tex:372 · p. 1345

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phenomenon 49.6: A maximum mass for a cold degenerate star49.6proposition 49.2: Ground-state pressure of the ideal Fermi gas49.2theorem 49.7: The Chandrasekhar mass49.7theorem 44.27: Newtonian correspondence of the field equations44.27proof : ch:08-compact-stars@proof-5proofphenomenon 83.1: Exclusion, and the lengths of the periods83.1theorem 40.5: Energy–momentum relation40.5phenomenon 49.8: The white-dwarf luminosity function has an edge49.8phenomenon 49.1: Matter at a billion kilograms per cubic metre49.1proof : ch:08-compact-stars@proof-2proofequation 49.7: eq:compact-lane-emden-mass49.7equation 49.3: eq:compact-ur-pressure49.3proposition 49.3: Lane–Emden form of hydrostatic equilibrium; restated from the stellar-structure chapter49.3proof : ch:08-compact-stars@proof-6proofdefinition 44.15: Dust44.15proposition 44.26: Newtonian limit of geodesic motion44.26proposition 44.4: Trace-reversed form44.4corollary 44.35: The field equations are essentially unique44.35phenomenon 49.16: Pulsars: clocks at nuclear density49.16phenomenon 49.14: A neutron star is observed being born49.14proposition 44.29: Linearized field equations44.29proof : ch:03-einstein-field-equations@proof-15proof

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typedirectionnode provenancewhere
cites The Maximum Mass of Ideal White Dwarfs derived parts/05-general-relativity-cosmology/08-compact-stars.tex:377
depends_on Ground-state pressure of the ideal Fermi gas declared parts/05-general-relativity-cosmology/08-compact-stars.tex:383
depends_on The Chandrasekhar mass declared parts/05-general-relativity-cosmology/08-compact-stars.tex:383
depends_on Newtonian correspondence of the field equations declared parts/05-general-relativity-cosmology/08-compact-stars.tex:383
proves ch:08-compact-stars@proof-5 declared parts/05-general-relativity-cosmology/08-compact-stars.tex:387