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arXiv · 1009.2877

Thermal Behaviour of Euclidean Stars

G. Govender·M. Govender·K. S. Govinder
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Abstract

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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G. Govender, M. Govender, K. S. Govinder. 2010-09-15. Thermal Behaviour of Euclidean Stars. https://doi.org/10.1142/s0218271810018049

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