On quasinormal modes for scalar perturbations of static spherically symmetric black holes in Nash embedding framework
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Publication:2364312
DOI10.1155/2017/9891231zbMath1366.83066arXiv1611.00430OpenAlexW3097999294WikidataQ59142228 ScholiaQ59142228MaRDI QIDQ2364312
Abraão J. S. Capistrano, R. G. G. Amorim, Sérgio C. Ulhoa
Publication date: 18 July 2017
Published in: Advances in High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1611.00430
Black holes (83C57) Semiclassical techniques, including WKB and Maslov methods applied to problems in quantum theory (81Q20)
Cites Work
- Classification of minimum global embeddings for nonrotating black holes
- Geometrical aspects on the dark matter problem
- On the existence of a static black hole on a brane
- The hierarchy problem and new dimensions at a millimeter
- The deformable universe
- The imbedding problem for Riemannian manifolds
- Stability and thermodynamics of brane black holes
- The embedding of Schwarzschild in braneworld
- The large \(N\) limit of superconformal field theories and supergravity
- Detection of gravitational waves from black holes: is there a window for alternative theories?
- On classical thermal stability of black holes with a dynamical extrinsic curvature
- Graviton time delay and a speed limit for small black holes in Einstein-Gauss-Bonnet theory
- The Higgs particle and higher-dimensional theories
- Embeddings for the Schwarzschild metric: classification and new results
- Quasinormal modes of Reissner–Nordström–anti-de Sitter black holes: Scalar, electromagnetic, and gravitational perturbations
- Stability of a Schwarzschild Singularity
- Isometric embedding of the spherically symmetric Stephani universe: Some explicit examples
- Large Mass Hierarchy from a Small Extra Dimension
- An Alternative to Compactification
- On the geometry of dark energy
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