The dynamical structure of the Einstein equations for a non-rotating star

DOI10.1007/BF00756964zbMath0773.35079OpenAlexW2044267874MaRDI QIDQ1801510

Giulio Magli

Publication date: 3 November 1993

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00756964

zbMATH Keywords

relativistic elasticityTolman-Oppenheimer-Volkhoff equations

Mathematics Subject Classification ID

Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) PDEs in connection with relativity and gravitational theory (35Q75)

Related Items (11)

Relating Material and Space-Time Metrics Within Relativistic Elasticity: A Dynamical Example ⋮ Conformal transformations in general relativistic elasticity ⋮ Unconstrained variational principle and canonical structure for relativistic elasticity ⋮ Tuning the properties of matter to any chosen dynamical behavior in cosmological models with elastic media ⋮ Kerr–Schild gravitational fields in matter and the Kerr-interior problem in general relativity ⋮ Erratum to: General spherically symmetric elastic stars in relativity ⋮ Anisotropic charged fluid spheres in D space–time dimensions ⋮ Analysing the elasticity difference tensor of general relativity ⋮ General spherically symmetric elastic stars in relativity ⋮ Generating elastic solutions of the Einstein field equations from the Schwarzschild vacuum solution ⋮ Cylindrically symmetric static solutions of the Einstein field equations for elastic matter

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