A microscopic description of black hole evaporation via holography
Abstract
Here, we propose a description of how a large, cold black hole (black zerobrane) in type IIA superstring theory evaporates into freely propagating D0branes, by solving the dual gauge theory quantitatively. The energy spectrum of emitted D0branes 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 D0branes, 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:

 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)
 Publication Date:
 Research Org.:
 Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
 Sponsoring Org.:
 USDOE
 OSTI Identifier:
 1416507
 Report Number(s):
 LLNLJRNL685083
Journal ID: ISSN 02182718; TRN: US1800944
 Grant/Contract Number:
 AC5207NA27344
 Resource Type:
 Accepted Manuscript
 Journal Name:
 International Journal of Modern Physics D
 Additional Journal Information:
 Journal Volume: 25; Journal Issue: 12; Journal ID: ISSN 02182718
 Publisher:
 World Scientific
 Country of Publication:
 United States
 Language:
 English
 Subject:
 79 ASTRONOMY AND ASTROPHYSICS; 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; string theory; black hole; quantum gravity
Citation Formats
Berkowitz, Evan, Hanada, Masanori, and Maltz, Jonathan. A microscopic description of black hole evaporation via holography. United States: N. p., 2016.
Web. doi:10.1142/S0218271816440028.
Berkowitz, Evan, Hanada, Masanori, & Maltz, Jonathan. A microscopic description of black hole evaporation via holography. United States. doi:10.1142/S0218271816440028.
Berkowitz, Evan, Hanada, Masanori, and Maltz, Jonathan. Tue .
"A microscopic description of black hole evaporation via holography". United States. doi:10.1142/S0218271816440028. https://www.osti.gov/servlets/purl/1416507.
@article{osti_1416507,
title = {A microscopic description of black hole evaporation via holography},
author = {Berkowitz, Evan and Hanada, Masanori and Maltz, Jonathan},
abstractNote = {Here, we propose a description of how a large, cold black hole (black zerobrane) in type IIA superstring theory evaporates into freely propagating D0branes, by solving the dual gauge theory quantitatively. The energy spectrum of emitted D0branes 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 D0branes, 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.},
doi = {10.1142/S0218271816440028},
journal = {International Journal of Modern Physics D},
number = 12,
volume = 25,
place = {United States},
year = {2016},
month = {7}
}
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