A microscopic description of black hole evaporation via holography
Volume
25
Pagination
1644002 - ?
Publisher
DOI
10.1142/s0218271816440028
Journal
International Journal of Modern Physics D
Issue
ISSN
0218-2718
Metadata
Show full item recordAbstract
We propose a description of how a large, cold black hole (black zero-brane) in type IIA superstring theory evaporates into freely propagating
D
0-branes, by solving the dual gauge theory quantitatively. The energy spectrum of emitted
D
0-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
D
0-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.
Authors
Berkowitz, E; Hanada, M; Maltz, JCollections
- Mathematics [1686]