THERMAL BEHAVIOR OF EUCLIDEAN STARS

DOI10.1142/S0218271810018049zbMath1204.85010arXiv1009.2877OpenAlexW2047756234MaRDI QIDQ3067215

M. Govender, G. Govender, Keshlan S. Govinder

Publication date: 20 January 2011

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

Full work available at URL: https://arxiv.org/abs/1009.2877

zbMATH Keywords

thermodynamicssheardissipative collapse

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) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Stability and instability of geophysical and astrophysical flows (76E20)

Related Items (11)

The role of pressure during shearing, dissipative collapse ⋮ Radiating stars with exponential Lie symmetries ⋮ Geodesic models generated by Lie symmetries ⋮ A general class of Euclidean stars ⋮ THE ROLE OF SHEAR IN DISSIPATIVE GRAVITATIONAL COLLAPSE ⋮ Generalized Euclidean stars with equation of state ⋮ SELF-GRAVITATING SPHERES OF ANISOTROPIC FLUID IN GEODESIC FLOW ⋮ Gravitational collapse for a radiating anisotropic fluid ⋮ Riccati equations for bounded radiating systems ⋮ Shearing radiative collapse with expansion and acceleration ⋮ Impact of anisotropic stresses during dissipative gravitational collapse

Cites Work

• Dissipative collapse in the presence of \(\Lambda \)
• THERMAL EVOLUTION OF A RADIATING ANISOTROPIC STAR WITH SHEAR
• A Riccati equation in radiative stellar collapse
• A causal model of radiating stellar collapse
• On Continued Gravitational Contraction
• Causal solutions for radiating stellar collapse

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