DYNAMICS OF VISCOUS DISSIPATIVE GRAVITATIONAL COLLAPSE: A FULL CAUSAL APPROACH

DOI10.1142/S0218271809014285zbMath1163.83356arXiv0804.3584OpenAlexW2003792914MaRDI QIDQ3629643

O. Troconis, E. Fuenmayor, Luis Herrera, Alicia Di Prisco

Publication date: 2 June 2009

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0804.3584

Mathematics Subject Classification ID

Space-time singularities, cosmic censorship, etc. (83C75) Galactic and stellar structure (85A15)

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Cites Work

• Stability and causality in dissipative relativistic fluids
• The gravitational field of a radiating and contracting spherically-symmetric body with heat flow
• Hyperbolic theories of dissipation: Why and when do we need them?
• Shear-free spherically symmetric spacetimes with an equation of state p = αρ
• THERMAL EVOLUTION OF A RADIATING ANISOTROPIC STAR WITH SHEAR
• THE INERTIA OF HEAT AND ITS ROLE IN THE DYNAMICS OF DISSIPATIVE COLLAPSE
• A Riccati equation in radiative stellar collapse
• The isotropic singularity in cosmology
• A causal model of radiating stellar collapse
• Heat waves
• Nonlinear shear‐free radiative collapse
• On Continued Gravitational Contraction
• The Thermodynamics of Irreversible Processes. III. Relativistic Theory of the Simple Fluid
• Causal solutions for radiating stellar collapse

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