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arxiv: 1610.08547 · v2 · pith:2ST5S4MInew · submitted 2016-10-26 · 🧮 math.DG · gr-qc· math.AP

Linear stability of Schwarzschild spacetime subject to axial perturbations

classification 🧮 math.DG gr-qcmath.AP
keywords linearizedschwarzschildconnection-leveleinsteinequationslinearmetricobject
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In this paper, we address the issue of linear stability of Schwarzschild space- time subject to certain axisymmetric perturbations. In particular, we prove that associ- ated solutions to the linearized vacuum Einstein equations centered at a Schwarzschild metric, with suitably regular initial data, decay to a linearized Kerr metric. Our method employs a complex line bundle interpretation applied to a connection-level object, allow- ing for direct analysis of this connection-level object by the linearized Einstein equations, in contrast with the recent breakthrough of Dafermos-Holzegel-Rodnianski.

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    Proves global nonlinear stability of subextremal Kerr black holes, with solutions settling to a nearby Kerr member at rate O(t_*^{-2-ε_K}) from initial data with O(r^{-1-ε0}) decay.