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Cited by 196

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(Anti-)evaporation of Schwarzschild–de Sitter black holes

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Bousso, Raphael, Hawking, Stephen W.·1998·Physical Review D

Abstract

We study the quantum evolution of black holes immersed in a de Sitter background space. For black holes whose size is comparable to that of the cosmological horizon, this process differs significantly from the evaporation of asymptotically flat black holes. Our model includes the one-loop effective action in the s-wave and large N approximation. Black holes of the maximal mass are in equilibrium. Unexpectedly, we find that nearly maximal quantum Schwarzschild--de Sitter black holes anti-evaporate. However, there is a different perturbative mode that leads to evaporation. We show that this mode will always be excited when a pair of cosmological holes nucleates.

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Research works printed but not linked: 9

  1. J. G. Russo, 1992, Phys. Lett. B, 292, 13, 10.1016/0370-2693(92)90601-Y · DOI · Paper page
  2. J. G. Russo, 1992, Phys. Rev. D, 46, 3444, 10.1103/PhysRevD.46.3444 · DOI · Paper page
  3. R. Bousso, 1997, Phys. Rev. Lett., 56, 7788
  4. H. Nariai, 1951, Sci. Rep. Res. Inst. Tohoku Univ. A, 35, 62
  5. P. Ginsparg, 1983, Nucl. Phys., B222, 245, 10.1016/0550-3213(83)90636-3 · DOI · Paper page
  6. J. D. Hayward, 1995, Phys. Rev. D, 52, 2239, 10.1103/PhysRevD.52.2239 · DOI
  7. S. Nojiri, 1997, Mod. Phys. Lett. A, 112, 2083, 10.1142/S0217732397002132 · DOI
  8. R. Bousso, 1995, Phys. Rev. D, 52, 5659, 10.1103/PhysRevD.52.5659 · DOI
  9. R. Bousso, 1997, Phys. Rev. D, 55, 3614, 10.1103/PhysRevD.55.3614 · DOI

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Metadata

Authors
Bousso, R., & Hawking, S. W.
Venue
Physical Review D
Published
1998-02-15
Volume
57
Issue
4
Pages
2436-2442
ISSN
  • 0556-2821 (ISSN-L)
  • 1089-4918
OpenAlex
W1998966260
Cited by
196
References
6
FWCI
7.52
Type
journal article
Language
en
Open access
green

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Bousso, R., & Hawking, S. W. (1998). (Anti-)evaporation of Schwarzschild–de Sitter black holes. Physical Review D. https://doi.org/10.1103/physrevd.57.2436

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