RADIATING GRAVITATIONAL COLLAPSE WITH SHEAR VISCOSITY AND BULK VISCOSITY

DOI10.1142/S0218271804005158zbMath1064.83051MaRDI QIDQ4832430

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Publication date: 4 January 2005

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

zbMATH Keywords

shear viscosityblack holegravitational collapsebulk viscosity

Mathematics Subject Classification ID

Space-time singularities, cosmic censorship, etc. (83C75) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Related Items (16)

Some anisotropic planar stellar models ⋮ Radiating shear-free gravitational collapse with charge ⋮ Static Axially Symmetric Models and Structure Scalars in Self-Interacting Brans–Dicke Gravity ⋮ Gravitational potential effects on shearing geodesic fluid solutions of Einstein's equations ⋮ Radiant gravitational collapse with anisotropy in pressures and bulk viscosity ⋮ Radiating stars with generalised Vaidya atmospheres ⋮ Dynamical analysis for cylindrical geometry in non-minimally coupled f(R,T) gravity ⋮ Causal thermodynamics of a gravitational collapse model for an anisotropic fluid with dissipative flows ⋮ A Riccati equation in radiative stellar collapse ⋮ THE ROLE OF SHEAR IN DISSIPATIVE GRAVITATIONAL COLLAPSE ⋮ Radiating gravitational collapse with shear viscosity revisited ⋮ Radiating gravitational collapse with an initial inhomogeneous energy density distribution ⋮ RADIATING GRAVITATIONAL COLLAPSE WITH SHEARING MOTION AND BULK VISCOSITY REVISITED ⋮ Gravitational collapse for a radiating anisotropic fluid ⋮ Mixed potentials in radiative stellar collapse ⋮ Shearing radiative collapse with expansion and acceleration

Cites Work

• A shearing non-adiabatic solution of Einstein's equations
• Shear-free spherically symmetric spacetimes with an equation of state p = αρ
• 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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