Extreme charged black holes in a braneworld with a cosmological constant

Ryotaku Suzuki, Tetsuya Shiromizu, Norihiro Tanahashi

Research output: Contribution to journalArticle

4 Citations (Scopus)

Abstract

Application of the AdS/CFT correspondence to the Randall-Sundrum models may predict that there is no static solution for black holes with a radius larger than the bulk curvature scale. When the black hole has an extremal horizon, however, the correspondence suggests that the black hole can stay static. We focus on the effects of cosmological constant on the brane on such extremal brane-localized black holes. We observe that the positive cosmological constant restricts the black hole size on the brane as in ordinary four-dimensional general relativity. The maximum black hole size differs from that in four-dimensional general relativity case due to the nonlinear term in the effective Einstein equation. In the negative cosmological constant case, we obtain an implication on the Newton constant in the Karch-Randall model.

Original languageEnglish
Article number085029
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume82
Issue number8
DOIs
Publication statusPublished - Oct 27 2010
Externally publishedYes

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relativity
Einstein equations
guy wires
newton
horizon
curvature
radii

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics
  • Physics and Astronomy (miscellaneous)

Cite this

Extreme charged black holes in a braneworld with a cosmological constant. / Suzuki, Ryotaku; Shiromizu, Tetsuya; Tanahashi, Norihiro.

In: Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 82, No. 8, 085029, 27.10.2010.

Research output: Contribution to journalArticle

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