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Charged brane-world black holes

Open access
Chamblin, Andrew, Reall, Harvey S., Shinkai, Hisa-aki, Shiromizu, Tetsuya·2001·Physical Review D

Abstract

We study charged brane-world black holes in the model of Randall and Sundrum in which our universe is viewed as a domain wall in asymptotically anti--de Sitter space. Such black holes can carry two types of ``charge,'' one arising from the bulk Weyl tensor and one from a gauge field trapped on the wall. We use a combination of analytical and numerical techniques to study how these black holes behave in the bulk. It has been shown that a Reissner-Nordstr\"om geometry is induced on the wall when only Weyl charge is present. However, we show that such solutions exhibit pathological features in the bulk. For more general charged black holes, our results suggest that the extent of the horizon in the fifth dimension is usually less than for an uncharged black hole that has the same mass or the same horizon radius on the wall.

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Metadata

Authors
Chamblin, A., Reall, H. S., Shinkai, H.-A., & Shiromizu, T.
Venue
Physical Review D
Published
2001-02-13
Volume
63
Issue
6
ISSN
  • 0556-2821 (ISSN-L)
  • 1089-4918
OpenAlex
W1967693859
Cited by
158
References
6
FWCI
10.78
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Charged brane-world black holes. https://app.cochat.ai/papers/10.1103/physrevd.63.064015
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Chamblin, A., Reall, H. S., Shinkai, H.-A., & Shiromizu, T. (2001). Charged brane-world black holes. Physical Review D. https://doi.org/10.1103/physrevd.63.064015

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