The DOI matches its Crossref record; 20 of the 20 references it cites were found in a registry or an index.
Entropy, area, and black hole pairs
Open accessAbstract
We clarify the relation between gravitational entropy and the area of horizons. We first show that the entropy of an extreme Reissner-Nordstr\"om black hole is zero, despite the fact that its horizon has nonzero area. Next, we consider the pair creation of extremal and nonextremal black holes. It is shown that the action which governs the rate of this pair creation is directly related to the area of the acceleration horizon and (in the nonextremal case) the area of the black hole event horizon. This provides a simple explanation of the result that the rate of pair creation of nonextreme black holes is enhanced by precisely the black hole entropy. Finally, we discuss black hole annihilation, and argue that Planck scale remnants are not sufficient to preserve unitarity in quantum gravity.
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Citations
Cites
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Volovik, G. E. (2009) · doi:10.1093/acprof:oso/9780199564842.001.0001 · Cited by 2,632
Charged AdS black holes and catastrophic holography
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The gravitational Hamiltonian, action, entropy and surface terms
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Tunnelling, temperature, and Taub-NUT black holes
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Metadata
- Authors
- Hawking, S. W., Horowitz, G. T., & Ross, S. F.
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 1995-04-15
- Volume
- 51
- Issue
- 8
- Pages
- 4302-4314
- ISSN
- 0556-2821 (ISSN-L)
- OpenAlex
- W2008341518
- Cited by
- 477
- References
- 20
- FWCI
- 26.29
- Type
- journal article
- Language
- en
- Open access
- green
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