Radiating collapse in the presence of anisotropic stresses

DOI10.1142/S0218271816500371zbMath1339.83056OpenAlexW2276499427MaRDI QIDQ2806279

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Publication date: 17 May 2016

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

Full work available at URL: https://doi.org/10.1142/s0218271816500371

zbMATH Keywords

gravitational collapseheat fluxEckartanisotropic stressescausal temperaturesstellar configuration

Mathematics Subject Classification ID

Black holes (83C57) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) 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) Equations of motion in general relativity and gravitational theory (83C10)

Related Items (3)

Dynamical forces and the influence of an equation of state on gravitational collapse ⋮ Complexity‐Free Anisotropic Solution of Buchdahl's Model and Energy Exchange Between Relativistic Fluids by Extended Gravitational Decoupling ⋮ Shear-free radiating collapse model via Karmarkar condition in f(R) gravity

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