Thermal Behaviour of Euclidean Stars

Details Thermal Behaviour of Euclidean Stars Thermal Behaviour of Euclidean Stars

2010-09-15

arxiv.org/abs/1009.2877v1

Int.J.Mod.Phys.D19:1773-1782,2010

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

10 pages, 3 figures

Scientific paper

10.1142/S0218271810018049

A recent study of dissipative collapse considered a contracting sphere in which the areal and proper radii are equal throughout its evolution. The interior spacetime was matched to the exterior Vaidya spacetime which generated a temporal evolution equation at the boundary of the collapsing sphere. We present a solution of the boundary condition which allows the study of the gravitational and thermodynamical behaviour of this particular radiating model.

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