Quasinormal modes for massless topological black holes
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An exact expression for the quasinormal modes of scalar perturbation on a massless topological black hole in four and higher dimensions is presented. The massive scalar field is nonminimally coupled to the curvature, and the horizon geometry is assumed to have a negative constant curvature.
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- Authors
- Aros, R., Martínez, C., Troncoso, R., & Zanelli, J.
- Affiliations
- Universidad Andrés Bello (CL)
- Centro de Estudios Científicos (CL)
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 2003-02-27
- Volume
- 67
- Issue
- 4
- ISSN
- 0556-2821 (ISSN-L)
- 1089-4918
- OpenAlex
- W2169781037
- Cited by
- 102
- References
- 37
- Citations by year
- 2026: 1 · 2024: 1 · 2022: 3 · 2021: 1 · 2019: 4 · 2018: 7 · 2017: 2 · 2016: 4 · 2014: 2 · 2013: 1 · 2012: 2
- FWCI
- 6.22
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- Americanae (AECID Library) (submittedVersion, other-oa)
- LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas) (submittedVersion, other-oa)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Noncommutative and Quantum Gravity Theories
- Keywords
- quasinormal modes, topological black holes, massless scalar field, scalar perturbations, higher-dimensional black holes, exact solutions
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