Resumen
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.
Idioma original | Inglés |
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Publicación | Physical Review D - Particles, Fields, Gravitation and Cosmology |
Volumen | 67 |
N.º | 4 |
DOI | |
Estado | Publicada - 2003 |
Publicado de forma externa | Sí |
Áreas temáticas de ASJC Scopus
- Física nuclear y de alta energía
- Física y astronomía (miscelánea)