Graviton emission in the bulk from a higher-dimensional Schwarzschild black hole

DOI10.1016/j.physletb.2006.02.030zbMath1247.83075arXivhep-th/0601126OpenAlexW2064510116MaRDI QIDQ454046

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

Publication date: 30 September 2012

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

Full work available at URL: https://arxiv.org/abs/hep-th/0601126

zbMATH Keywords

evaporationSchwarzschild black hole\((4+n)\)-dimensional non-rotating black holes

Mathematics Subject Classification ID

Black holes (83C57) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (8)

Influence of a brane tension on phantom and massive scalar field emission ⋮ Hawking radiation power equations for black holes ⋮ VALIDITY OF EMPARAN–HOROWITZ-MYERS ARGUMENT IN HAWKING RADIATION INTO MASSLESS SPIN-2 FIELDS ⋮ Hawking emission from quantum gravity black holes ⋮ Electromagnetic quasinormal modes of \(D\)-dimensional black holes ⋮ Angular profile of particle emission from a higher-dimensional black hole: analytic results ⋮ Black Holes at the Large Hadron Collider ⋮ Signatures of extra dimensions in gravitational waves

Cites Work

• Black holes in higher dimensional space-times
• Symmetric-tensor eigenspectrum of the Laplacian on n-spheres
• An Alternative to Compactification
• BLACK HOLES IN THEORIES WITH LARGE EXTRA DIMENSIONS: A REVIEW
• A Master Equation for Gravitational Perturbations of Maximally Symmetric Black Holes in Higher Dimensions

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