On the symmetries of equilibrium stellar models

DOI10.1098/rsta.1992.0072zbMath0770.76075OpenAlexW2011554302MaRDI QIDQ4697070

Lee Lindblom

Publication date: 29 June 1993

Published in: Philosophical Transactions of the Royal Society of London. Series A: Physical and Engineering Sciences (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1098/rsta.1992.0072

zbMATH Keywords

Einstein equationsspatial symmetryequilibrium solutionsNewtonian theoryself-gravitating fluids

Mathematics Subject Classification ID

General theory of rotating fluids (76U05) Galactic and stellar structure (85A15) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Research exposition (monographs, survey articles) pertaining to fluid mechanics (76-02)

Related Items (7)

On the spherical symmetry of static stellar models ⋮ A geometric approach to the classification of the equilibrium shapes of self-gravitating fluids ⋮ (In)finite extent of stationary perfect fluids in Newtonian theory ⋮ Uniqueness of static, isotropic low-pressure solutions of the Einstein-Vlasov system ⋮ Rotating elastic bodies in Einstein gravity ⋮ Ground states of self-gravitating elastic bodies ⋮ Multi-body spherically symmetric steady states of Newtonian self-gravitating elastic matter

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