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Paper detail

Thermal Behaviour of Euclidean Stars

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.

preprint2010arXivOpen access
G. GovenderM. GovenderK. S. Govinder
gr-qc
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G. GovenderM. GovenderK. S. Govinder

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