NON-ADIABATIC GRAVITATIONAL COLLAPSE OF A SUPERDENSE STAR

DOI10.1142/S0218271810018098zbMath1204.85016MaRDI QIDQ3067223

Ramesh Tikekar, Sanjay B. Sarwe

Publication date: 20 January 2011

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

zbMATH Keywords

general relativityneutron stars

Mathematics Subject Classification ID

Black holes (83C57) Space-time singularities, cosmic censorship, etc. (83C75) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Classical and relativistic thermodynamics (80A10) Galactic and stellar structure (85A15) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (4)

Collapsing shear-free radiating fluid spheres ⋮ Radiating stars with exponential Lie symmetries ⋮ Space-time inhomogeneity, anisotropy and gravitational collapse ⋮ Riccati equations for bounded radiating systems

Cites Work

• On most general exact solution for Vaidya-Tikekar isentropic superdense star
• Hyperbolic theories of dissipation: Why and when do we need them?
• Exact model for a relativistic star
• PARABOLOIDAL SPACE–TIMES AND RELATIVISTIC MODELS OF STRANGE STARS
• 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
• Radiating relativistic matter in geodesic motion
• Collapse of a radiating star
• More about collapse of a radiating star
• General solution for a relativistic star
• A causal model of radiating stellar collapse
• Radiating gravitational collapse before relaxation
• Exact solutions for the Tikekar superdense star
• RADIATING COLLAPSE WITH VANISHING WEYL STRESSES
• Heat waves
• SHEAR-FREE RADIATING COLLAPSE AND CONFORMAL FLATNESS
• On Continued Gravitational Contraction

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