Gravitational collapse: a case for thermal relaxation

DOI10.1023/A:1018862910233zbMath0915.53040arXivgr-qc/9710125MaRDI QIDQ1289215

K. Appert

Publication date: 13 June 1999

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

Full work available at URL: https://arxiv.org/abs/gr-qc/9710125

zbMATH Keywords

relaxation timecollapsing spheresmass loss of stars

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Applications of differential geometry to physics (53Z05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Related Items (12)

RADIATING COLLAPSE WITH VANISHING WEYL STRESSES ⋮ Radiating shear-free gravitational collapse with charge ⋮ Dynamics of uniformally collapsing system and the horizon formation ⋮ Shear-free radiating collapse model via Karmarkar condition in f(R) gravity ⋮ Dissipative collapse of a Karmarkar star ⋮ A general class of Euclidean stars ⋮ RELATIVISTIC GRAVITATIONAL COLLAPSE IN COMOVING COORDINATES: THE POST-QUASISTATIC APPROXIMATION ⋮ Generating black holes in 4D Einstein–Gauss–Bonnet gravity ⋮ Matching conditions in locally rotationally symmetric spacetimes and radiating stars ⋮ Causal solutions for radiating stellar collapse ⋮ THERMAL EVOLUTION OF A RADIATING ANISOTROPIC STAR WITH SHEAR ⋮ Impact of anisotropic stresses during dissipative gravitational collapse

Cites Work

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• An equation of state for radiating dissipative spheres in general relativity
• Gravitational waves in general relativity, VII. Waves from axi-symmetric isolated system
• Some models of anisotropic spheres in general relativity
• Radiating gravitational collapse before relaxation
• Junction conditions and the propagation of isometries in general relativity
• Static Solutions of Einstein's Field Equations for Spheres of Fluid

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