Bulk versus brane emissivities of photon fields: for the case of higher-dimensional Schwarzschild phase
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Publication:881347
DOI10.1016/j.nuclphysb.2007.01.002zbMath1117.83377arXivhep-th/0610089OpenAlexW2091120328MaRDI QIDQ881347
Publication date: 22 May 2007
Published in: Nuclear Physics. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/hep-th/0610089
Black holes (83C57) String and superstring theories in gravitational theory (83E30) Quantization of the gravitational field (83C45)
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Cites Work
- Unnamed Item
- Condition for the superradiance modes in higher-dimensional rotating black holes with multiple angular momentum parameters
- Particle creation by black holes
- Emissivities for the various graviton modes in the background of the higher-dimensional black hole
- Absorption and emission spectra of an higher-dimensional Reissner-Nordström black hole
- Bulk versus brane in the absorption and emission: 5d rotating black hole case
- Black holes in higher dimensional space-times
- Quasinormal modes of Reissner–Nordström–anti-de Sitter black holes: Scalar, electromagnetic, and gravitational perturbations
- Stability of a Schwarzschild Singularity
- String Theory
- An Alternative to Compactification
- Master Equations for Perturbations of Generalised Static Black Holes with Charge in Higher Dimensions
- BLACK HOLES IN THEORIES WITH LARGE EXTRA DIMENSIONS: A REVIEW
- A Master Equation for Gravitational Perturbations of Maximally Symmetric Black Holes in Higher Dimensions
- Black Holes Radiate Mainly on the Brane
- Hawking radiation of the brane-localized graviton from a (4 + n )-dimensional black hole