de Sitter spacetime: effects of metric perturbations on geodesic motion

被引:0
|
作者
Donato Bini
Giampiero Esposito
Andrea Geralico
机构
[1] Istituto per le Applicazioni del Calcolo “M. Picone,Physics Department and ICRA
[2] ” CNR,undefined
[3] ICRA,undefined
[4] University of Rome “La Sapienza”,undefined
[5] INFN—Sezione di Firenze,undefined
[6] Polo Scientifico,undefined
[7] INFN,undefined
[8] Sezione di Napoli,undefined
[9] Complesso Universitario di Monte S. Angelo,undefined
[10] University of Rome “LaSapienza”,undefined
来源
General Relativity and Gravitation | 2012年 / 44卷
关键词
de Sitter spacetime; Gravitational perturbations; Teukolsky equation; Liouvillian solutions;
D O I
暂无
中图分类号
学科分类号
摘要
Gravitational perturbations of the de Sitter spacetime are investigated using the Regge–Wheeler formalism. The set of perturbation equations is reduced to a single second order differential equation of the Heun-type for both electric and magnetic multipoles. The solution so obtained is used to study the deviation from an initially radial geodesic due to the perturbation. The spectral properties of the perturbed metric are also analyzed. Finally, gauge- and tetrad-invariant first-order massless perturbations of any spin are explored following the approach of Teukolsky. The existence of closed-form, i.e. Liouvillian, solutions to the radial part of the Teukolsky master equation is discussed.
引用
收藏
页码:467 / 490
页数:23
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