Asymptotic tails of massive scalar fields in Schwarzschild background

dc.creatorKoyama, Hiroko
dc.creatorTomimatsu, Akira
dc.date2001-03-23
dc.date2001-05-04
dc.date.accessioned2026-07-07T08:33:22Z
dc.date.available2026-07-07T08:33:22Z
dc.descriptionWe investigate the asymptotic tail behavior of massive scalar fields in Schwarzschild background. It is shown that the oscillatory tail of the scalar field has the decay rate of $t^{-5/6}$ at asymptotically late times, and the oscillation with the period $2π/m$ for the field mass $m$ is modulated by the long-term phase shift. These behaviors are qualitatively similar to those found in nearly extreme Reissner-Nordström background, which are discussed in terms of a resonant backscattering due to the space-time curvature.
dc.description21 pages, 2 figures, accepted for publication in Phys.Rev.D
dc.identifierhttps://arxiv.org/abs/gr-qc/0103086
dc.identifierhttp://arxiv.org/abs/gr-qc/0103086
dc.identifierPhys.Rev. D64 (2001) 044014
dc.identifierdoi:10.1103/PhysRevD.64.044014
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/139103
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleAsymptotic tails of massive scalar fields in Schwarzschild background
dc.typetext

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