Asymptotic power-law tails of massive scalar fields in Reissner-Nordström background

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dc.creatorKoyama, Hiroko
dc.creatorTomimatsu, Akira
dc.date2000-12-06
dc.date2000-12-22
dc.date.accessioned2026-07-07T08:33:22Z
dc.date.available2026-07-07T08:33:22Z
dc.descriptionWe investigate dominant late-time tail behaviors of massive scalar fields in nearly extreme Reissner-Nordström background. It is shown that the oscillatory tail of the scalar fields has the decay rate of $t^{-5/6}$ at asymptotically late times. The physical mechanism by which the asymptotic $t^{-5/6}$ tail yields and the relation between the field mass and the time scale when the tail begins to dominate, are discussed in terms of resonance backscattering due to spacetime curvature.
dc.description18 pages, 1 figure, accepted for publication in Physical Review D
dc.identifierhttps://arxiv.org/abs/gr-qc/0012022
dc.identifierhttp://arxiv.org/abs/gr-qc/0012022
dc.identifierPhys.Rev. D63 (2001) 064032
dc.identifierdoi:10.1103/PhysRevD.63.064032
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/139102
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleAsymptotic power-law tails of massive scalar fields in Reissner-Nordström background
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