A microscopic description of black hole evaporation via holography
Journal Article
·
· International Journal of Modern Physics D
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Stanford Univ., Stanford, CA (United States); Kyoto Univ., Kyoto (Japan)
- Stanford Univ., Stanford, CA (United States); Univ. of California, Berkeley, CA (United States)
Here, we propose a description of how a large, cold black hole (black zero-brane) in type IIA superstring theory evaporates into freely propagating D0-branes, by solving the dual gauge theory quantitatively. The energy spectrum of emitted D0-branes is parametrically close to thermal when the black hole is large. The black hole, while initially cold, gradually becomes an extremely hot and stringy object as it evaporates. As it emits D0-branes, its emission rate speeds up and it evaporates completely without leaving any remnant. Hence this system provides us with a concrete holographic description of black hole evaporation without information loss.
- Research Organization:
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Sponsoring Organization:
- USDOE
- Grant/Contract Number:
- AC52-07NA27344
- OSTI ID:
- 1416507
- Report Number(s):
- LLNL-JRNL-685083; TRN: US1800944
- Journal Information:
- International Journal of Modern Physics D, Vol. 25, Issue 12; ISSN 0218-2718
- Publisher:
- World ScientificCopyright Statement
- Country of Publication:
- United States
- Language:
- English
Cited by: 12 works
Citation information provided by
Web of Science
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