RADIATING GRAVITATIONAL COLLAPSE WITH SHEAR REVISITED

DOI10.1142/S0218271803003463zbMath1079.83017OpenAlexW1994471270MaRDI QIDQ5700001

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Publication date: 27 October 2005

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

Full work available at URL: https://doi.org/10.1142/s0218271803003463

zbMATH Keywords

radiationheat flowshearGravitational collapse

Mathematics Subject Classification ID

Black holes (83C57)

Related Items (8)

Radiating shear-free gravitational collapse with charge ⋮ Radiating stars with exponential Lie symmetries ⋮ Analysis of the boundary condition and equation of state in radiating stars ⋮ THE ROLE OF SHEAR IN DISSIPATIVE GRAVITATIONAL COLLAPSE ⋮ Generalized Euclidean stars with equation of state ⋮ Radiating gravitational collapse with shear viscosity revisited ⋮ RADIATING GRAVITATIONAL COLLAPSE WITH SHEARING MOTION AND BULK VISCOSITY REVISITED ⋮ Shearing radiative collapse with expansion and acceleration

Cites Work

• A generalization of the concept of adiabatic index for non-adiabatic systems
• A shearing non-adiabatic solution of Einstein's equations
• Collapse of a radiating star
• Energy conditions for an imperfect fluid
• Spherical Symmetry and Mass-Energy in General Relativity. I. General Theory
• ‘Newtonian’ Time in General Relativity

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