The DOI matches its Crossref record; 2 of the 2 references it cites were found in a registry or an index.
Effect of self-interaction on charged black hole radiance
Open accessAbstract
Abstract We extend our previous analysis of the modification of the spectrum of black hole radiance due to the simplest and probably most quantitatively important back-reaction effect, that is self-gravitational interaction, to the case of charged holes. As anticipated, the corrections are small for low-energy radiation when the hole is well away from extremality, but become qualitatively important near extremality. A notable result is that radiation which could leave the hole with mass and charge characteristic of a naked singularity, predicted in the usual approximation of fixed space-time geometry, is here suppressed. We discuss the nature of our approximations, and show how they work in a simpler electromagnetic analogue problem.
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Citations
Cites
Particle creation by black holes
Hawking, S. W. (1975) · Communications In Mathematical Physics · doi:10.1007/bf02345020 · Cited by 13,106
Self-interaction correction to black hole radiance
Kraus, P., & Wilczek, F. (1995) · Nuclear Physics B · doi:10.1016/0550-3213(94)00411-7 · Cited by 594
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Cited by
Hot halos and galactic glasses (carbonado)
Anninos, D., Anous, T., Barandes, J., Denef, F., & Gaasbeek, B. (2012) · Journal of High Energy Physics · doi:10.1007/jhep01(2012)003 · Cited by 39
Metadata
- Authors
- Kraus, P., & Wilczek, F.
- Venue
- Nuclear Physics B
- Publisher
- Elsevier BV
- Published
- 1995-03
- Volume
- 437
- Issue
- 1
- Pages
- 231-242
- ISSN
- 0550-3213 (ISSN-L)
- OpenAlex
- W1970736407
- Cited by
- 350
- References
- 2
- FWCI
- 3.38
- Type
- journal article
- Language
- en
- Open access
- green
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