Symmetries of the gravitational scattering in the absence of peeling

被引:2
|
作者
Geiller, Marc [1 ]
Laddha, Alok [2 ]
Zwikel, Celine [3 ]
机构
[1] Univ Lyon, ENS Lyon, CNRS, Lab Phys, F-69342 Lyon, France
[2] SIPCOT IT Pk, Chennai Math Inst, H1, Kelambakkam 603103, India
[3] Perimeter Inst Theoret Phys, 31 Caroline St North, Waterloo, ON N2L 2Y5, Canada
来源
JOURNAL OF HIGH ENERGY PHYSICS | 2024年 / 12期
关键词
Classical Theories of Gravity; Gauge Symmetry; RELATIVISTIC KEPLER-PROBLEM; GENERAL-RELATIVITY; ASYMPTOTIC SYMMETRIES; WAVE BURSTS; FIELDS; NULL; RADIATION; BEHAVIOR; MEMORY; MODES;
D O I
10.1007/JHEP12(2024)081
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
The symmetries of the gravitational scattering are intimately tied to the symmetries which preserve asymptotic flatness at null infinity. In Penrose's definition of asymptotic flatness, a central role is played by the notion of asymptotic simplicity and the ensuing peeling behavior which dictates the decay rate of the Weyl tensor. However, there is now accumulating evidence that in a generic gravitational scattering the peeling property is broken, so that the spacetime is not asymptotically-flat in the usual sense. These obstructions to peeling can be traced back to the existence of universal radiative low frequency observables called "tails to the displacement memory". As shown by Saha, Sahoo and Sen, these observables are uniquely fixed by the initial and final momenta of the scattering objects, and are independent of the details of the scattering. The universality of these tail modes is the statement of the classical logarithmic soft graviton theorem. Four-dimensional gravitation scattering therefore exhibits a rich infrared interplay between tail to the memory, loss of peeling, and universal logarithmic soft theorems.In this paper we study the solution space and the asymptotic symmetries for logarithmically-asymptotically-flat spacetimes. These are defined by a polyhomogeneous expansion of the Bondi metric which gives rise to a loss of peeling, and represent the classical arena which can accommodate a generic gravitational scattering containing tails to the memory. We show that while the codimension-two generalized BMS charges are sensitive to the loss of peeling at I\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$ \mathcal{I} $$\end{document}+, the flux is insensitive to the fate of peeling. Due to the tail to the memory, the soft superrotation flux contains a logarithmic divergence whose coefficient is the quantity which is conserved in the scattering by virtue of the logarithmic soft theorem. In our analysis we also exhibit new logarithmic evolution equations and flux-balance laws, whose presence suggests the existence of an infinite tower of subleading logarithmic soft graviton theorems.
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页数:38
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