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The Case Against Smooth Null Infinity II: A Logarithmically Modified Price's Law

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arxiv 2105.08084 v2 pith:TOK76YNQ submitted 2021-05-17 gr-qc hep-thmath-phmath.APmath.DGmath.MP

classification gr-qchep-thmath-phmath.APmath.DGmath.MP
keywords mathcalnullinfinitysmoothalongasymptoticsconstantdata
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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 $i^0$ derived therein translates into logarithmic corrections at leading order to the well-known Price's law asymptotics near $i^+$. This suggests that the non-smoothness of $\mathcal{I}^+$ is physically measurable. More precisely, we consider the linear wave equation $\Box_g \phi=0$ on a fixed Schwarzschild background ($M>0$), and we show the following: If one imposes conformally smooth initial data on an ingoing null hypersurface (extending to $\mathcal{H}^+$ and terminating at $\mathcal{I}^-$) and vanishing data on $\mathcal{I}^-$ (this is the no incoming radiation condition), then the precise leading-order asymptotics of the solution $\phi$ are given by $r\phi|_{\mathcal{I}^+}=C u^{-2}\log u+\mathcal{O}(u^{-2})$ along future null infinity, $\phi|_{r=R>2M}=2C\tau^{-3}\log\tau+\mathcal{O}(\tau^{-3})$ along hypersurfaces of constant $r$, and $\phi|_{\mathcal{H}^+}=2Cv^{-3}\log v+\mathcal{O}(v^{-3})$ along the event horizon. Moreover, the constant $C$ is given by $C=4M I_0^{(\mathrm{past})}[\phi]$, where $I_0^{(\mathrm{past})}[\phi]:=\lim_{u\to -\infty} r^2\partial_u(r\phi_{\ell=0})$ is the past Newman--Penrose constant of $\phi$ on $\mathcal{I}^-$. Thus, the precise late-time asymptotics of $\phi$ are completely determined by the early-time behaviour of the spherically symmetric part of $\phi$ near $\mathcal{I}^-$. Similar results are obtained for polynomially decaying timelike boundary data. The paper uses methods developed by Angelopoulos--Aretakis--Gajic and is essentially self-contained.

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Cited by 3 Pith papers

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  1. The Energy-Momentum-News Complex near Future Null Infinity

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    A Carroll-covariant energy-momentum-news complex at future null infinity yields Ward identities that generalise the Bondi loss equations, with an anomalous Carroll boost.

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    For asymptotically regular spacetimes, parity-time reversal symmetry of the leading and subleading initial data implies the Weyl scalars Psi2 and Psi1 peel at null infinity with rates 1/r^3 and 1/r^4.

  3. Twisting asymptotically-flat spacetimes

    gr-qc 2025-11 conditional novelty 6.0 of 10

    Twisting asymptotically-flat spacetimes are brought into a generalized Bondi gauge with finite radial expansion, producing new flux-balance laws, Carroll-boost symmetries, and finite supertranslated Kerr–Taub–NUT metrics.

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