Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
Scientific paper
2000-11-14
Phys.Rev.D64:024029,2001
Astronomy and Astrophysics
Astrophysics
General Relativity and Quantum Cosmology
16 pages RevTeX, 5 EPS figures added
Scientific paper
10.1103/PhysRevD.64.024029
In terms of the Painlev{\'e}-Gullstrand-Lema{\^\i}tre coordinates a rather general scenario for the gravitational collapse of an object and the subsequent formation of a horizon is described by a manifestly $C^\infty$-metric. For a 1+1 dimensional model of the collapse the leading contributions to the Bogoliubov coefficients are calculated explicitely and the Hawking temperature is recovered. But depending on the particular dynamics of the collapse the final state represents either evaporation or anti-evaporation. The generalization of the calculation to 3+1 dimensions is outlined and possible implications are addressed. PACS-numbers: 04.70.Dy, 04.70.-s, 04.62.+v.
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