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Slowly rotating charged Gauss-Bonnet black holes in AdS spaces

2007/11/06 by Hyeong-Chan Kim, Rong-Gen Cai · 1 citation
Physics and Astronomy · #Astrophysical Phenomena and Observations #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #hep-th

paper · pdf · doi:10.1103/physrevd.77.024045

published as Phys.Rev.D77:024045,2008 · 10 pages, 3 figures

arxiv created 2007/11/06 · openalex publication_date 2008/01/28 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/30

Abstract

Rotating charged Gauss-Bonnet black hole solutions in higher dimensional (d>4), asymptotically anti-de Sitter spacetime are obtained in the small angular momentum limit. The angular momentum, magnetic dipole moment, and the gyromagnetic ratio of the black holes are calculated and it turns out that the Gauss-Bonnet term does not affect the gyromagnetic ratio.

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