Scalar emission in the bulk in a rotating black hole background

DOI10.1016/j.physletb.2007.09.050zbMath1246.83109arXiv0709.0241OpenAlexW2030380761MaRDI QIDQ446835

Simon Creek, O. Efthimiou, Kyriakos Tamvakis, Panagiota Kanti

Publication date: 8 September 2012

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

Full work available at URL: https://arxiv.org/abs/0709.0241

zbMATH Keywords

rotating black holes

Mathematics Subject Classification ID

Black holes (83C57)

Related Items (8)

Greybody factor for a static spherically symmetric black hole with non-linear electrodynamics ⋮ Influence of a brane tension on phantom and massive scalar field emission ⋮ Greybody factors for Myers–Perry black holes ⋮ Hawking emission from quantum gravity black holes ⋮ Angular profile of particle emission from a higher-dimensional black hole: analytic results ⋮ Black Holes at the Large Hadron Collider ⋮ Greybody factor for a rotating Bardeen black hole by perfect fluid dark matter ⋮ Exact greybody factors for the brane scalar field of five-dimensional rotating black holes

Cites Work

• Condition for the superradiance modes in higher-dimensional rotating black holes with multiple angular momentum parameters
• Hawking radiation from a \((4+n)\)-dimensional rotating black hole on the brane
• Particle creation by black holes
• Bulk versus brane in the absorption and emission: 5d rotating black hole case
• Black holes in higher dimensional space-times
• Spherical harmonics
• An Alternative to Compactification
• Hawking radiation of the brane-localized graviton from a (4 + n )-dimensional black hole
• TeV-scale black hole lifetimes in extra-dimensional Lovelock gravity

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