Microscopic origin of the Bekenstein-Hawking entropy
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The statement that 'a black hole has no hair' is now known to be not always true.
“In addition, the well-known statement that 'a black hole has no hair'-i.e., from a distance all black holes with the same charge and angular momentum look essentially alike - is now known to be not always true 91 -93 .”
From Ultimate physical limits to computation (2000) · cites this paper as [93]
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- Authors
- Strominger, A., & Vafa, C.
- Affiliations
- University of California, Santa Barbara (US)
- Harvard University (US)
- ORCID
- Vafa, Cumrun
- Venue
- Physics Letters B
- Publisher
- Elsevier BV
- Published
- 1996-06
- Volume
- 379
- Issue
- 1-4
- Pages
- 99-104
- ISSN
- 0370-2693 (ISSN-L)
- OpenAlex
- W2130491267
- Cited by
- 3,072
- References
- 12
- Citations by year
- 2026: 121 · 2025: 174 · 2024: 131 · 2023: 152 · 2022: 105 · 2021: 110 · 2020: 132 · 2019: 140 · 2018: 84 · 2017: 105 · 2016: 108 · 2015: 86 · 2014: 84 · 2013: 105 · 2012: 95
- FWCI
- 83.83
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Physics Letters B (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- Digital Access to Scholarship at Harvard (DASH) (Harvard University) (submittedVersion, cc-by)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
- Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Statistical Mechanics and Entropy
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Particle physics theoretical and experimental studies
- Keywords
- Bekenstein-Hawking entropy, black hole entropy, BPS solitons, bound states, microscopic entropy, string theory
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