Late-time tail of a coupled scalar field in the background of a black hole with a global monopole
arXiv:gr-qc/0511098 · doi:10.1142/S0217732308023888
Abstract
Using the technique of spectral decomposition, we investigated the late-time tails of massless and massive coupled scalar fields in the background of a black hole with a global monopole. We found that due to existence of the coupling between the scalar and gravitational fields, the massless scalar field decay faster at timelike infinity , and so does the massive one in the intermediate late time. But the asymptotically late-time tail for the massive scalar field is not affected and its decay rate still is .
12 pages, A corrected version to be appeared in MPLA
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- Gravitational field of a slowly rotating black hole with phantom global monopole
- Dynamical evolution of the electromagnetic perturbation with Weyl corrections
- Maxwell quasinormal modes on a global monopole Schwarzschild-anti-de Sitter black hole with Robin boundary conditions
- Dirac quasinormal modes of power-Maxwell charged black holes in Rastall gravity
- Late-time evolution of Dirac field around Schwarzschild-quintessence black hole
- Qusinormal oscillations and late-time tail of massless scalar perturbations of a magnetized black hole in Rastall gravity
- Dynamical evolution of phantom scalar perturbation in the background of Schwarzschild black String spacetime
- Effects of global monopole on critical behaviors and microstructure of charged AdS black holes
- Nonlinear tails of massive scalar fields around a black hole