arXiv · 1909.06733
The linear stability of the Schwarzschild spacetime in the harmonic gauge: even part
Abstract
In this paper we study the even part of the linear stability of the Schwarzschild spacetime as a continuation of [22]. By taking the harmonic gauge, we prove that the energy decays at a rate $\tau^{-2+}$ for the solution of the linearized Einstein equation after subtracting its spherically symmetric part. We further show that the spherically symmetric part converges to a linear combination of two special solutions. One is the gauge-fixed mass change solution [19]. The other is the deformation tensor of a stationary one form, which solves the tensorial wave equation. As a key ingredient, we prove that the solutions of the tensorial wave equation converge to this stationary one form up to a scalar multiplication.
Explore related subjects
Keep this discovery
Pei-Ken Hung. 2019-09-15. The linear stability of the Schwarzschild spacetime in the harmonic gauge: even part. https://arxiv.org/abs/1909.06733
Cite the original work for its findings. Save a collection to share your selection of sources.