A variational principle for the axisymmetric stability of rotating relativistic stars

DOI10.1088/0264-9381/33/18/185007zbMath1349.83019arXiv1606.00859OpenAlexW3105805281MaRDI QIDQ2832540

Kartik Prabhu, Robert M. Wald, Joshua S. Schiffrin

Publication date: 11 November 2016

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1606.00859

zbMATH Keywords

stabilityvariational principlegeneral relativityfluid stars

Mathematics Subject Classification ID

Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Dynamical systems in other branches of physics (quantum mechanics, general relativity, laser physics) (37N20) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Exact solutions to problems in general relativity and gravitational theory (83C15)

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