Embedding condition describing shearing, dissipative collapse

DOI10.1016/j.aop.2021.168458zbMath1464.85002OpenAlexW3155361873MaRDI QIDQ2037406

M. Govender, Sunil D. Maharaj, Wesley Govender, Kevin P. Reddy

Publication date: 1 July 2021

Published in: Annals of Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/j.aop.2021.168458

zbMATH Keywords

spherical symmetryshearcompact objectsKarmarkar condition

Mathematics Subject Classification ID

Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15)

Related Items (2)

Shearing, dissipative collapse influenced by an equation of state ⋮ Radiant gravitational collapse with anisotropy in pressures and bulk viscosity

Cites Work

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• Stability and horizon formation during dissipative collapse
• Impact of anisotropic stresses during dissipative gravitational collapse
• A different approach to anisotropic spherical collapse with shear and heat radiation
• Shearing radiative collapse with expansion and acceleration
• RADIATING GRAVITATIONAL COLLAPSE WITH SHEARING MOTION AND BULK VISCOSITY REVISITED
• THERMAL EVOLUTION OF A RADIATING ANISOTROPIC STAR WITH SHEAR
• Dynamical instability for non-adiabatic spherical collapse
• A causal model of radiating stellar collapse
• Dissipative collapse of a Karmarkar star
• Mixed potentials in radiative stellar collapse
• THE ROLE OF SHEAR IN DISSIPATIVE GRAVITATIONAL COLLAPSE

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