Spherically symmetric radiating solution with heat flow in general relativity
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Publication:3992332
DOI10.1063/1.529722zbMath0753.76204OpenAlexW2053010680MaRDI QIDQ3992332
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Publication date: 13 August 1992
Published in: Journal of Mathematical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1063/1.529722
Schwarzschild solutioncollapsing spherespherically symmetric shear-free fluid configurationVaidya's pure radiation field
Related Items (13)
Relativistic model for radiating star ⋮ Collapsing shear-free radiating fluid spheres ⋮ Radiating stars with generalised Vaidya atmospheres ⋮ Some new exact solutions with finite central parameters and uniform radial motion of sound ⋮ Horizon-free gravitational collapse of radiating fluid sphere ⋮ Collapsing shear-free perfect fluid spheres with heat flow ⋮ An exact solution of perfect fluid in isotropic coordinates, compatible with relativistic modeling of star ⋮ Diffusive and dynamical radiating stars with realistic equations of state ⋮ Relativistic model of radiating massive fluid sphere ⋮ Gravitational collapse without a remnant ⋮ THERMAL EVOLUTION OF A RADIATING ANISOTROPIC STAR WITH SHEAR ⋮ The gravitational field of a radiating and contracting spherically-symmetric body with heat flow ⋮ Relativistic collapsing radiating stars
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