Non-adiabatic collapse of a quasi-spherical radiating star

Details Non-adiabatic collapse of a quasi-spherical radiating star Non-adiabatic collapse of a quasi-spherical radiating star

2003-10-16

arxiv.org/abs/gr-qc/0310080v1

Gen.Rel.Grav.37:215-223,2005

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

8 Latex pages, No figures, Revtex style

Scientific paper

10.1007/s10714-005-0010-6

A model is proposed of a collapsing quasi-spherical radiating star with matter content as shear-free isotropic fluid undergoing radial heat-flow with outgoing radiation. To describe the radiation of the system, we have considered both plane symmetric and spherical Vaidya solutions. Physical conditions and thermodynamical relations are studied using local conservation of momentum and surface red-shift. We have found that for existence of radiation on the boundary, pressure on the boundary is not necessary.

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