Support of dS/CFT correspondence from perturbations of three-dimensional spacetime
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Publication:1601276
DOI10.1016/S0370-2693(02)02039-7zbMath0995.81136arXivhep-th/0204030OpenAlexW2015246852MaRDI QIDQ1601276
Publication date: 25 June 2002
Published in: Physics Letters. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/hep-th/0204030
Related Items (11)
Quasinormal modes of \(D\)-dimensional de Sitter spacetime ⋮ Charged scalar quasi-normal modes for linearly charged dilaton-Lifshitz solutions ⋮ Strong cosmic censorship in higher-dimensional Reissner-Nordström-de Sitter spacetime ⋮ Dirac and Klein–Gordon–Fock equations in Grumiller’s spacetime ⋮ QUASINORMAL MODES AND LATE-TIME TAILS IN THE BACKGROUND OF SCHWARZSCHILD BLACK HOLE PIERCED BY A COSMIC STRING: SCALAR, ELECTROMAGNETIC AND GRAVITATIONAL PERTURBATIONS ⋮ Evolution of massive fields around a black hole in Hořava gravity ⋮ Area Quantization in Quasi-Extreme Black Holes ⋮ Absorption and quasinormal modes of classical fields propagating on 3D and 4D de Sitter spacetime ⋮ Quasinormal modes from potentials surrounding the charged-dilaton black hole ⋮ Electromagnetic quasinormal modes of \(D\)-dimensional black holes ⋮ A model of quantum gravity with emergent spacetime
Cites Work
- Central charges in the canonical realization of asymptotic symmetries: An example from three dimensional gravity
- Statistical entropy of de Sitter space
- Large \(N\) field theories, string theory and gravity
- Black hole in three-dimensional spacetime
- Comments on black holes in string theory
- The (2 + 1)-dimensional black hole
- Quasi-normal modes of stars and black holes
- Quasinormal modes of Reissner-Nordström anti-de Sitter black holes
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