Soft Hair on Black Holes
Open accessAbstract
It has recently been shown that Bondi-van der Burg-Metzner-Sachs supertranslation symmetries imply an infinite number of conservation laws for all gravitational theories in asymptotically Minkowskian spacetimes. These laws require black holes to carry a large amount of soft (i.e., zero-energy) supertranslation hair. The presence of a Maxwell field similarly implies soft electric hair. This Letter gives an explicit description of soft hair in terms of soft gravitons or photons on the black hole horizon, and shows that complete information about their quantum state is stored on a holographic plate at the future boundary of the horizon. Charge conservation is used to give an infinite number of exact relations between the evaporation products of black holes which have different soft hair but are otherwise identical. It is further argued that soft hair which is spatially localized to much less than a Planck length cannot be excited in a physically realizable process, giving an effective number of soft degrees of freedom proportional to the horizon area in Planck units.
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One key aspect of this class of models is to give prominence to hair degrees of freedom on the horizon which are approximately conserved (non-)gravitational charges.
“One key aspect of this class of models is to give prominence to hair degrees of freedom on the horizon which are essentially (approximately) conserved (non-)gravitational charges”
From Holographic spacetime, black holes and quantum error correcting codes: a review (2022) · cites this paper as [261]
Cites
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“That would require, at a minimum, a detailed understanding of the information flow out of black holes as well as a derivation of the Hawking-Bekenstein area-entropy law [2, 3, 47].”
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“That would require, at a minimum, a detailed understanding of the information flow out of black holes as well as a derivation of the Hawking-Bekenstein area-entropy law [2, 3, 47].”
BackgroundSelf-citationBreakdown of predictability in gravitational collapse
Hawking, S. W. (1976) · Physical Review D · doi:10.1103/physrevd.14.2460 · Cited by 2,554 · see citing works
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“The plethora of proposals for new physics that might be associated with obtaining this Page curve (including [3, 7–39]) were thus all properly viewed as speculative and contained at least some optimistic extrapolation or ad hoc ingredient.”
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Self-citationHolographic spacetime, black holes and quantum error correcting codes: a review
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- Authors
- Hawking, S. W., Perry, M. J., & Strominger, A.
- Affiliations
- University of Cambridge (GB)
- Harvard University (US)
- Venue
- Physical Review Letters
- Publisher
- American Physical Society (APS)
- Published
- 2016-06-06
- Volume
- 116
- Issue
- 23
- Pages
- 231301-231301
- ISSN
- 0031-9007 (ISSN-L)
- 1079-7114
- OpenAlex
- W2225733786
- Cited by
- 764
- References
- 3
- Citations by year
- 2026: 28 · 2025: 61 · 2024: 57 · 2023: 56 · 2022: 57 · 2021: 74 · 2020: 89 · 2019: 102 · 2018: 80 · 2017: 100 · 2016: 59 · 2015: 1
- FWCI
- 54.94
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Licence
- Locations
- Physical Review Letters (publishedVersion)
- PubMed (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- Digital Access to Scholarship at Harvard (DASH) (Harvard University) (submittedVersion, cc-by)
- Queen Mary Research Online (Queen Mary University of London) (submittedVersion)
- arXiv (Cornell University)
- Funders
- Science and Technology Facilities Council
- National Science Foundation (1205550)
- Cynthia and George Mitchell Foundation
- Topics
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Relativity and Gravitational Theory
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysical Phenomena and Observations
- Keywords
- soft hair, black holes, soft gravitons, soft photons, holographic plates, black hole evaporation, charge conservation, horizon area
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