The Case Against Smooth Null Infinity II: A Logarithmically Modified Price's Law
arXiv:2105.08084 · doi:10.4310/ATMP.2022.v26.n10.a6
Abstract
In this paper, we expand on results from our previous paper "The Case Against Smooth Null Infinity I: Heuristics and Counter-Examples" [1] by showing that the failure of "peeling" (and, thus, of smooth null infinity) in a neighbourhood of derived therein translates into logarithmic corrections at leading order to the well-known Price's law asymptotics near . This suggests that the non-smoothness of is physically measurable. More precisely, we consider the linear wave equation on a fixed Schwarzschild background (), and we show the following: If one imposes conformally smooth initial data on an ingoing null hypersurface (extending to and terminating at ) and vanishing data on (this is the no incoming radiation condition), then the precise leading-order asymptotics of the solution are given by along future null infinity, along hypersurfaces of constant , and along the event horizon. Moreover, the constant is given by , where is the past Newman--Penrose constant of on . Thus, the precise late-time asymptotics of are completely determined by the early-time behaviour of the spherically symmetric part of near . Similar results are obtained for polynomially decaying timelike boundary data. The paper uses methods developed by Angelopoulos--Aretakis--Gajic and is essentially self-contained.
34 pages, 3 figures
References in corpus (3)
Cited by in corpus (5)
- Local supersymmetry and the square roots of Bondi-Metzner-Sachs supertranslations
- On the Relation Between Asymptotic Charges, the Failure of Peeling and Late-time Tails
- The Case Against Smooth Null Infinity III: Early-Time Asymptotics for Higher -Modes of Linear Waves on a Schwarzschild Background
- The Case Against Smooth Null Infinity V: Early-Time Asymptotics of Linearised Gravity Around Schwarzschild for Fixed Spherical Harmonic Modes
- Scattering for wave equations with sources close to the lightcone and prescribed radiation fields