Proposal of a gauge-invariant treatment of l=0,1-mode perturbations on Schwarzschild Background Spacetime
arXiv:2102.00830 · doi:10.1088/1361-6382/ac03f9
Abstract
A gauge-invariant treatment of the monopole- () and dipole () modes in linear perturbations of the Schwarzschild background spacetime is proposed. Through this gauge-invariant treatment, we derived the solutions to the linearized Einstein equation for these modes with a generic matter field. In the vacuum case, these solutions include the Kerr parameter perturbations in the odd modes and the additional mass parameter perturbations of the Schwarzschild mass in the even modes. The linearized version of Birkhoff's theorem is also confirmed in a gauge-invariant manner. In this sense, our proposal is reasonable.
(v1) 10 pages, no figure; (v2) 16 pages, Section 2 is added for the explanation of our previous works, Additional explanations are added, references are added and re-organized; (v3) Some explanations are added, Typos are corrected
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Cited by in corpus (6)
- Backreaction of scalar waves on black holes at low frequencies
- Backreaction of Mass and Angular Momentum Accretion on Black Holes: General Formulation of the Metric Perturbations and Application to the Blandford-Znajek Process
- Comparing a gauge-invariant formulation and a "conventional complete gauge-fixing approach" for mode perturbations on the Schwarzschild background spacetime
- Gauge-invariant perturbation theory on the Schwarzschild background spacetime Part I : -- Formulation and odd-mode perturbations
- Gauge-invariant perturbation theory on the Schwarzschild background spacetime Part II: -- Even-mode perturbations
- Gauge-invariant perturbation theory on the Schwarzschild background spacetime Part III: -- Realization of exact solutions