Relativistic model of radiating massive fluid sphere

DOI10.1007/s10509-010-0320-3zbMath1195.85011OpenAlexW2098327490MaRDI QIDQ989697

R. N. Mehta, Neeraj Pant, B. C. Tewari

Publication date: 23 August 2010

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10509-010-0320-3

zbMATH Keywords

general relativityquasarsupernova burst

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15) Stability and instability of geophysical and astrophysical flows (76E20)

Related Items (4)

Relativistic modelling of a superdense star containing a charged perfect fluid ⋮ Some new exact solutions with finite central parameters and uniform radial motion of sound ⋮ Horizon-free gravitational collapse of radiating fluid sphere ⋮ A well-behaved class of charged analogue of Durgapal solution

Cites Work

• Relativistic model for radiating star
• Radiating fluid spheres in general relativity
• Quasi-spherical solution with heat flux and non-adiabatic collapse of radiating star
• Conformally-flat metric representing a radiating fluid ball
• Spherically symmetric radiating solution with heat flow in general relativity
• RADIATING COLLAPSE WITH VANISHING WEYL STRESSES
• SHEAR-FREE RADIATING COLLAPSE AND CONFORMAL FLATNESS
• Static Solutions of Einstein's Field Equations for Spheres of Fluid
• Nonstatic Solutions of Einstein's Field Equations for Spheres of Fluids Radiating Energy
• ‘Newtonian’ Time in General Relativity

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