The linear stability of the Schwarzschild solution to gravitational perturbations in the generalised wave gauge
arXiv:1810.01337 · doi:10.1007/s40818-019-0069-0
Abstract
We prove in this paper that the Schwarzschild famiily of black holes are linearly stable as a family of solutions to the system of equations that result from expressing the Einstein vacuum equations in a generalised wave gauge. In particular we improve on our recent work \cite{Johnsonlinstabschwarzold} by modifying the generalised wave gauge employed therein so as to establish asymptotic flatness of the associated linearised system. The result thus complements the seminal work \cite{DHRlinstabschwarz} of Dafermos-Holzegel-Rodnianski in a similar vein as to how the work \cite{LRstabmink} of Lindblad-Rodnianski complemented that of Christodoulou-Klainerman \cite{CKstabmink} in establishing the nonlinear stability of the Minkowski space. This paper is the content of the authors PhD thesis.
arXiv commentRemoved the statement of the conjecture regarding the nonlinear stability of Schwarzschild due to Dafermos--Holzegel--Rodnianski so as to remove a text overlap
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Cited by in corpus (12)
- The linear stability of Reissner-Nordström spacetime: the full subextremal range
- The linear stability of the Schwarzschild solution to gravitational perturbations in the generalised wave gauge
- A sharp version of Price's law for wave decay on asymptotically flat spacetimes
- The linear stability of Reissner-Nordström spacetime for small charge
- Sharp decay estimates for massless Dirac fields on a Schwarzschild background
- The Stable Trapping Phenomenon for Black Strings and Black Rings and its Obstructions on the Decay of Linear Waves
- Price's law for spin fields on a Schwarzschild background
- Boundedness and decay for the Teukolsky system of spin on Reissner-Nordström spacetime: the case
- Decay estimates for the massless Vlasov equation on Schwarzschild spacetimes
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- On the link between the Maxwell and linearised Einstein equations on Schwarzschild
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