The gravitational field of a radiating and contracting spherically-symmetric body with heat flow

DOI10.1023/A:1001991223754zbMath0959.83034OpenAlexW1652592130MaRDI QIDQ1596256

Dirk Schäfer, Hubert F. M. Goenner

Publication date: 11 February 2001

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1023/a:1001991223754

zbMATH Keywords

heat flowgravitational radiation

Mathematics Subject Classification ID

General relativity (83C99) Classical and relativistic thermodynamics (80A10)

Related Items

Conformally flat collapsing stars in \(f(R)\) gravity ⋮ RADIATING COLLAPSE WITH VANISHING WEYL STRESSES ⋮ Spherical doubly warped spacetimes for radiating stars and cosmology ⋮ Charged anisotropic collapsing stars with heat flux in \(f(R)\) gravity ⋮ GRAVITATIONAL COLLAPSE OF SELF-SIMILAR AND SHEAR-FREE FLUID WITH HEAT FLOW ⋮ Diffusive and dynamical radiating stars with realistic equations of state ⋮ Space-time inhomogeneity, anisotropy and gravitational collapse ⋮ Gravitational collapse without a remnant ⋮ DYNAMICS OF VISCOUS DISSIPATIVE GRAVITATIONAL COLLAPSE: A FULL CAUSAL APPROACH ⋮ A class of conformally flat solutions for systems undergoing radiative gravitational collapse

Cites Work

• Thermodynamics of a model of nonadiabatic spherical gravitational collapse
• Radiating collapse solutions
• Collapse of a radiating star
• More about collapse of a radiating star
• Energy conditions for an imperfect fluid
• Spherically symmetric radiating solution with heat flow in general relativity
• A causal model of radiating stellar collapse
• The Large Scale Structure of Space-Time
• ‘Newtonian’ Time in General Relativity

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