Radiation equations for black holes

Details Radiation equations for black holes Radiation equations for black holes

2005-11-18

arxiv.org/abs/hep-th/0511183v1

Phys.Lett.B634:456-464,2006

Physics

High Energy Physics

High Energy Physics - Theory

16 pages, 1 figure. Latex 2.09. Figure PNG

Scientific paper

10.1016/j.physletb.2006.02.012

It has been shown in the previous paper that the metric in the semiclassical region of the collapse spacetime is expressed purely kinematically through the Bondi charges. Here the Bondi charges are expressed through this metric by calculating the vacuum radiation against its background. The result is closed equations for the metric and the Bondi charges. Notably, there is a nonvanishing flux of the vacuum-induced matter charge.

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