The Case Against Smooth Null Infinity II: A Logarithmically Modified Price's Law
Lionor M. A. Kehrberger

TL;DR
This paper demonstrates that Price's law asymptotics near future null infinity are modified by logarithmic terms due to non-smoothness at spatial infinity, with the leading behavior determined by initial data and the Newman-Penrose constant.
Contribution
It establishes the presence of logarithmic corrections to Price's law in Schwarzschild spacetime, linking late-time decay to initial data and the Newman-Penrose constant.
Findings
Logarithmic corrections appear in Price's law asymptotics.
Late-time behavior is determined by initial data near past null infinity.
Results are applicable to polynomially decaying boundary data.
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…
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Taxonomy
TopicsAdvanced Mathematical Physics Problems · Black Holes and Theoretical Physics · Cosmology and Gravitation Theories
