2021
DOI: 10.1007/s10455-021-09789-y
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Conformal scattering theory for the linearized gravity fields on Schwarzschild spacetime

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Cited by 3 publications
(14 citation statements)
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“…The result of Hörmander was extended for the scalar wave equation by Nicolas [19] with the following minor modifications: the C 1 -metric, the continuous coefficients of the derivatives of the first order and the terms of order zero have locally L ∞ -coefficients. We refer [6,15,21,24] for…”
Section: Appendix Amentioning
confidence: 99%
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“…The result of Hörmander was extended for the scalar wave equation by Nicolas [19] with the following minor modifications: the C 1 -metric, the continuous coefficients of the derivatives of the first order and the terms of order zero have locally L ∞ -coefficients. We refer [6,15,21,24] for…”
Section: Appendix Amentioning
confidence: 99%
“…The Goursat problem is an important step to construct the conformal scattering theory for the field equations in the asymptotic simple and flat spacetimes (in detail see [10,21] for the construction of the theory). In related work, the wellposedness of the Goursat problem and conformal scattering theories for the Regge-Wheeler and Zerilli equations in Schwarzschild spacetime have been obtained by Pham [24].…”
Section: Introductionmentioning
confidence: 99%
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“…In particular, the conformal scattering theory (i.e. the geometric scattering theory) has been studied extensively from the early works by Friedlander [25][26][27][28][29], Baez et al [8], Hörmander [37] to recent ones by Mason and Nicolas [49], Joudioux [41,42], Nicolas [59], Mokdad [53,54], Taujanskas [72] and Pham [63,65].…”
Section: Introductionmentioning
confidence: 99%
“…Continuing this program, Mokdad [53,54] constructed explicitly the conformal scattering theories for the Maxwell and Dirac equations on the static exterior and dynamic interior of Reissner-Nordström de Sitter spacetimes, respectively. On the other hand, Pham [63] constructed conformal scattering theories for the scalar Reeger-Wheeler and Zerelli equations arising from the linearized gravity fields and the spin ±2 Teukolsky equations. This is the first step to obtain the conformal scattering theory for the linearized gravity fields on the Schwarzschild spacetime which is spherical symmetric.…”
Section: Introductionmentioning
confidence: 99%