White dwarfs with anisotropic pressure in post-Newtonian gravity

DOI10.1023/A:1001548624783zbMath0944.76075OpenAlexW1641068876MaRDI QIDQ1300522

E. S. Corchero

Publication date: 20 September 2000

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1023/a:1001548624783

zbMATH Keywords

equilibrium configurationsneutron starswhite dwarfslocal anisotropycondition for equilibriummass above Chandrasekhar limitpost-Newtonian gravity

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Compressible fluids and gas dynamics (76N99)

Related Items (3)

Charged fluid sphere in bimetric general theory of relativity ⋮ Energy content of a collapsing sphere with f(R) gravity ⋮ The Weyl tensor and equilibrium configurations of self-gravitating fluids

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