The role of pressure during shearing, dissipative collapse

DOI10.1007/S10773-012-1221-8zbMath1255.83090OpenAlexW2020523030MaRDI QIDQ1930587

Yanyan Li

Publication date: 11 January 2013

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

Full work available at URL: https://doi.org/10.1007/s10773-012-1221-8

zbMATH Keywords

thermodynamicsgeneral relativityradiating stars

Mathematics Subject Classification ID

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) Exact solutions to problems in general relativity and gravitational theory (83C15) Equations of motion in general relativity and gravitational theory (83C10) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Stability and instability of geophysical and astrophysical flows (76E20) Radiative transfer in astronomy and astrophysics (85A25)

Related Items (6)

Some anisotropic planar stellar models ⋮ Thermal convection in a Brinkman-Darcy-Kelvin-Voigt fluid with a generalized Maxwell-Cattaneo law ⋮ Radiating stars with exponential Lie symmetries ⋮ THE ROLE OF THE ELECTROMAGNETIC FIELD IN DISSIPATIVE COLLAPSE ⋮ THE ROLE OF SHEAR IN DISSIPATIVE GRAVITATIONAL COLLAPSE ⋮ Impact of anisotropic stresses during dissipative gravitational collapse

Cites Work

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• THERMAL EVOLUTION OF A RADIATING ANISOTROPIC STAR WITH SHEAR
• A Riccati equation in radiative stellar collapse
• EXPANSION-FREE CAVITY EVOLUTION: SOME EXACT ANALYTICAL MODELS
• SPHERICAL COLLAPSE WITH HEAT FLOW AND WITHOUT HORIZON
• On Continued Gravitational Contraction

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