Thermodynamics for radiating shells in anti-de Sitter space-time

Details Thermodynamics for radiating shells in anti-de Sitter space-time Thermodynamics for radiating shells in anti-de Sitter space-time

2003-02-11

arxiv.org/abs/gr-qc/0302038v1

Phys.Lett.B557:7-11,2003

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

9 pages, 2 figures, PLB style

Scientific paper

10.1016/S0370-2693(03)00185-0

A thermodynamical description for the quasi-static collapse of radiating, self-gravitating spherical shells of matter in anti-de Sitter space-time is obtained. It is shown that the specific heat at constant area and other thermodynamical quantities may diverge before a black hole has eventually formed. This suggests the possibility of a phase transition occurring along the collapse process. The differences with respect to the asymptotically flat case are also highlighted.

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