Slowly rotating dilaton black hole in anti-de Sitter spacetime

Journal Article · Mon Oct 15 00:00:00 EDT 2007 · Physical Review. D, Particles Fields

DOI:https://doi.org/10.1103/PHYSREVD.76.087504· OSTI ID:21032521

Ghosh, Tanwi; SenGupta, Soumitra ^[1]

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1. Department of Theoretical Physics, Indian Association for the Cultivation of Science, Jadavpur, Calcutta-700 032 (India)

A rotating dilaton black hole solution for asymptotically anti-de Sitter spacetime is obtained in the small angular momentum limit with an appropriate combination of three Liouville-type dilaton potentials. The angular momentum, magnetic dipole moment, and the gyromagnetic ratio of such a black hole are determined for arbitrary values of the dilaton-electromagnetic coupling parameter.

• OSTI ID: 21032521
• Journal Information: Physical Review. D, Particles Fields, Vol. 76, Issue 8; Other Information: DOI: 10.1103/PhysRevD.76.087504; (c) 2007 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 0556-2821
• Country of Publication: United States
• Language: English

Related Subjects

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
ANGULAR MOMENTUM
BLACK HOLES
COSMOLOGICAL MODELS
COSMOLOGY
COUPLING
ELECTROMAGNETISM
GYROMAGNETIC RATIO
MAGNETIC DIPOLE MOMENTS
MATHEMATICAL SOLUTIONS
POTENTIALS
SPACE-TIME