Published March 23, 2006
| Version v1
Journal article
Radiation equations for black holes
Creators
- 1. Lebedev Physical Institute, and Lebedev Research Center in Physics, Leninsky Prospect 53, 119991 Moscow (Russian Federation)
Description
It has been shown in [G.A. Vilkovisky, hep-th/0511182] 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
Additional details
Identifiers
- DOI
- 10.1016/j.physletb.2006.02.012;
- arXiv
- arXiv:hep-th/0511183v1;
- PII
- S0370-2693(06)00166-3;
Publishing Information
- Journal Title
- Physics Letters. Section B
- Journal Volume
- 634
- Journal Issue
- 5-6
- Journal Page Range
- p. 456-464
- ISSN
- 0370-2693
- CODEN
- PYLBAJ
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 38029066
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- BLACK HOLES; EQUATIONS; MATTER; SEMICLASSICAL APPROXIMATION; SPACE-TIME
- Descriptors DEC
- APPROXIMATIONS; CALCULATION METHODS
Optional Information
- Copyright
- Copyright (c) 2006 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.