Quasinormal modes of D3-brane black holes
Open accessAbstract
We investigate a method to evaluate quasinormal modes of D3-brane black holes by wave interpretation of fields on a D3-brane based on Feynman's spacetime approach. We perturbatively solve the wave equation which describes propagation of a dilaton wave in a bulk space and its interaction with the D3-brane. The condition obtained for the quasinormal modes is qualitatively equivalent to that evaluated in the usual scattering of the dilaton in the black three-brane spacetime in the corresponding supergravity description.
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- Authors
- Kurita, Y., & Sakagami, M.-A.
- Affiliations
- Kyoto University (JP)
- Venue
- Physical Review D
- Publisher
- American Physical Society (APS)
- Published
- 2003-01-08
- Volume
- 67
- Issue
- 2
- ISSN
- 0556-2821 (ISSN-L)
- 1089-4918
- OpenAlex
- W2964219930
- Cited by
- 29
- References
- 34
- Citations by year
- 2022: 3 · 2019: 1 · 2018: 1 · 2016: 1 · 2014: 1
- FWCI
- 3.38
- 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)
- ePrints Soton (University of Southampton) (submittedVersion)
- Topics
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Particle physics theoretical and experimental studies
- Physical Sciences › Physics and Astronomy › Atomic and Molecular Physics, and Optics › Quantum Electrodynamics and Casimir Effect
- Keywords
- quasinormal modes, wave equation, D3-branes, supergravity, perturbation solution
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