Causal solutions for radiating stellar collapse
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Publication:5935181
DOI10.1016/S0375-9601(01)00190-6zbMath0982.85001MaRDI QIDQ5935181
M. Govender, Keshlan S. Govinder
Publication date: 20 June 2001
Published in: Physics Letters. A (Search for Journal in Brave)
Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar dynamics (85A05)
Related Items (21)
RADIATING COLLAPSE WITH VANISHING WEYL STRESSES ⋮ First integrals for charged perfect fluid distributions ⋮ Shearing, dissipative collapse influenced by an equation of state ⋮ Static Axially Symmetric Models and Structure Scalars in Self-Interacting Brans–Dicke Gravity ⋮ Non-adiabatic gravitational collapse in f(R,T) gravity with Karmarkar condition for anisotropic fluid ⋮ Radiating fluid sphere immersed in an anisotropic atmosphere ⋮ Shear-free radiating collapse model via Karmarkar condition in f(R) gravity ⋮ Dissipative collapse of a Karmarkar star ⋮ Collapsing shear-free perfect fluid spheres with heat flow ⋮ Causal thermodynamics of a gravitational collapse model for an anisotropic fluid with dissipative flows ⋮ A general class of Euclidean stars ⋮ Axially and reflection symmetric systems and structure scalars in \(f(R,T)\) gravity ⋮ THE ROLE OF SHEAR IN DISSIPATIVE GRAVITATIONAL COLLAPSE ⋮ Junction conditions for composite matter in higher dimensions ⋮ Dissipative collapse in the presence of \(\Lambda \) ⋮ THERMAL BEHAVIOR OF EUCLIDEAN STARS ⋮ DYNAMICS OF VISCOUS DISSIPATIVE GRAVITATIONAL COLLAPSE: A FULL CAUSAL APPROACH ⋮ Quasi-homologous evolution of relativistic stars ⋮ THERMAL EVOLUTION OF A RADIATING ANISOTROPIC STAR WITH SHEAR ⋮ Impact of anisotropic stresses during dissipative gravitational collapse ⋮ The influence of an equation-of-state during radiative collapse
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