theorem 49.7 The Chandrasekhar mass

open in the book · parts/05-general-relativity-cosmology/08-compact-stars.tex:437 · p. 1345

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theorem 49.7: The Chandrasekhar mass49.7equation 49.7: eq:compact-lane-emden-mass49.7equation 49.3: eq:compact-ur-pressure49.3proposition 49.2: Ground-state pressure of the ideal Fermi gas49.2proposition 49.3: Lane–Emden form of hydrostatic equilibrium; restated from the stellar-structure chapter49.3phenomenon 49.6: A maximum mass for a cold degenerate star49.6proof : ch:08-compact-stars@proof-6proofproposition 49.5: White-dwarf mass–radius relation49.5phenomenon 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 31.13: eq:fluid-hydrostatic31.13proposition 52.1: Hydrostatic equilibrium of a self-gravitating sphere52.1theorem 52.6: Lane–Emden equation52.6proof : ch:08-compact-stars@proof-3prooftheorem 44.27: Newtonian correspondence of the field equations44.27proof : ch:08-compact-stars@proof-5proof

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typedirectionnode provenancewhere
depends_on eq:compact-lane-emden-mass declared parts/05-general-relativity-cosmology/08-compact-stars.tex:456
depends_on eq:compact-ur-pressure declared parts/05-general-relativity-cosmology/08-compact-stars.tex:456
depends_on Ground-state pressure of the ideal Fermi gas declared parts/05-general-relativity-cosmology/08-compact-stars.tex:456
depends_on Lane–Emden form of hydrostatic equilibrium; restated from the stellar-structure chapter declared parts/05-general-relativity-cosmology/08-compact-stars.tex:456
depends_on A maximum mass for a cold degenerate star declared parts/05-general-relativity-cosmology/08-compact-stars.tex:383
proves ch:08-compact-stars@proof-6 declared parts/05-general-relativity-cosmology/08-compact-stars.tex:460