A Scattering Theory for Linearised Gravity on the Exterior of the Schwarzschild Black Hole I: The Teukolsky Equations
arXiv:2007.13658 · doi:10.1007/s00220-022-04372-3
Abstract
We construct a scattering theory for the spin Teukolsky equations on the exterior of the Schwarzschild spacetime, as a first step towards developing a scattering theory for the linearised Einstein equations in double null gauge. This is done by exploiting a physical-space version of the Chandrasekhar transformation used by Dafermos, Holzegel and Rodnianski in [arxiv:1601.06467] to prove the linear stability of the Schwarzschild solution. We also address the Teukolsky-Starobinsky correspondence and construct an isomorphism between scattering data for the and Teukolsky equations. This will allow us to state an additional mixed scattering statement for a pair of curvature components satisfying the spin and Teukolsky equations and connected via the Teukolsky-Starobinsky identities, completely determining the radiating degrees of freedom of solutions to the linearised Einstein equations.
83 pages, 4 figures
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- The non-linear stability of the Schwarzschild family of black holes
- The Case Against Smooth Null Infinity IV: Linearised Gravity Around Schwarzschild -- An Overview
- Peeling for tensorial wave equations on Schwarzschild spacetime
- The Case Against Smooth Null Infinity V: Early-Time Asymptotics of Linearised Gravity Around Schwarzschild for Fixed Spherical Harmonic Modes
- Conformal Scattering of Maxwell Potentials
- Conformal scattering theories for tensorial wave equations on Schwarzschild spacetime