Gauge-invariant perturbation theory on the Schwarzschild background spacetime Part II: -- Even-mode perturbations
arXiv:2110.13512 · doi:10.3390/universe11020042
Abstract
This is the Part II paper of our series of papers on a gauge-invariant perturbation theory on the Schwarzschild background spacetime. After reviewing our general framework of the gauge-invariant perturbation theory and the proposal on the gauge-invariant treatments for mode perturbations on the Schwarzschild background spacetime in the Part I paper [K.~Nakamura, arXiv:2110.13508 [gr-qc]], we examine the linearized Einstein equations for even-mode perturbations. We discuss the strategy to solve the linearized Einstein equations for these even-mode perturbations including modes. Furthermore, we explicitly derive the mode solutions to the linearized Einstein equations in both the vacuum and the non-vacuum cases. We show that the solutions for mode perturbations includes the additional Schwarzschild mass parameter perturbation, which is physically reasonable. Then, we conclude that our proposal of the resolution of the -mode problem is physically reasonable due to the realization of the additional Schwarzschild mass parameter perturbation and the Kerr parameter perturbation in the Part I paper.
arXiv comment34 pages, no figure, The Part II paper of the full paper version of the previous short papers arXiv:2102.00830v3[gr-qc] (v1); references are corrected. (v2); 33 pages, no figure, some explanations are added (v3); minor revision in explanations (v4); minor revision (v5)
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