Condition for the superradiance modes in higher-dimensional rotating black holes with multiple angular momentum parameters

DOI10.1016/j.physletb.2005.06.012zbMath1247.83097arXivhep-th/0504139OpenAlexW2080415764MaRDI QIDQ451739

Eylee Jung, Sung Hoon Kim, Dae Kil Park

Publication date: 23 September 2012

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/hep-th/0504139

zbMATH Keywords

higher-dimensional rotating black holes

Mathematics Subject Classification ID

Black holes (83C57)

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ENTANGLEMENT DEGRADATION IN THE PRESENCE OF (4 + n)-DIMENSIONAL SCHWARZSCHILD BLACK HOLE, Bulk versus brane in the absorption and emission: 5d rotating black hole case, Bulk versus brane emissivities of photon fields: for the case of higher-dimensional Schwarzschild phase, Quasinormal modes and stability of higher dimensional rotating black holes under massive scalar perturbations, Extension of non-minimal derivative coupling theory and Hawking radiation in black-hole spacetime, Scalar emission in the bulk in a rotating black hole background, Asymptotic quasinormal frequencies of brane-localized black hole, Analytic explanation of the strong spin-dependent amplification in Hawking radiation from rotating black holes, Emissivities for the various graviton modes in the background of the higher-dimensional black hole

Cites Work

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