THERMAL EVOLUTION OF A RADIATING ANISOTROPIC STAR WITH SHEAR
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Publication:3430408
DOI10.1142/S0218271806008760zbMath1119.85005arXivgr-qc/0509088MaRDI QIDQ3430408
M. Govender, Nolene F. Naidu, Keshlan S. Govinder
Publication date: 21 March 2007
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/gr-qc/0509088
Related Items (32)
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Cites Work
- A generalization of the concept of adiabatic index for non-adiabatic systems
- Gravitational collapse: a case for thermal relaxation
- Spherically symmetric radiating solution with heat flow in general relativity
- A causal model of radiating stellar collapse
- Radiating gravitational collapse before relaxation
- Spherical Symmetry and Mass-Energy in General Relativity. I. General Theory
- GRAVITATIONAL COLLAPSE OF SELF-SIMILAR AND SHEAR-FREE FLUID WITH HEAT FLOW
- On Continued Gravitational Contraction
- Causal solutions for radiating stellar collapse
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