Decay Rates for Spherical Scalar Waves in the Schwarzschild Geometry
Johann Kronthaler
TL;DR
The paper provides a rigorous analysis of late-time decay for a scalar field in Schwarzschild geometry, focusing on spherically symmetric initial data. It constructs an integral spectral representation using Jost solutions of the Regge-Wheeler Schrödinger equation and derives precise small-frequency expansions to analyze the Green's function kernel. The main result proves exact decay rates of $| ext{φ}(t)| \,\lerac{c}{t^3}$ in general and $| ext{φ}(t)| \,\\lerac{c}{t^4}$ for momentarily static data, showing these are optimal, and discusses extension to $l eq 0$ where Price's law predicts $t^{-2l-3}$ and $t^{-2l-4}$. These findings solidify Price's heuristic decay predictions in a rigorous framework and lay groundwork for broader stability analyses in black hole spacetimes.
Abstract
The Cauchy problem is considered for the scalar wave equation in the Schwarzschild geometry. Using an integral spectral representation we derive the exact decay rate for solutions of the Cauchy problem with spherical symmetric initial data, which is smooth and compactly supported outside the event horizon.
