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Autores principales: Floch, Bruno Le, LeFloch, Philippe G.
Formato: Preprint
Publicado: 2024
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Acceso en línea:https://arxiv.org/abs/2402.17598
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author Floch, Bruno Le
LeFloch, Philippe G.
author_facet Floch, Bruno Le
LeFloch, Philippe G.
contents To construct asymptotically-Euclidean Einstein's initial data sets, we introduce the localized seed-to-solution method, which projects from approximate to exact solutions of the Einstein constraints. The method enables us to glue together initial data sets in multiple asymptotically-conical regions, and in particular construct data sets that exhibit the gravity shielding phenomenon, specifically that are localized in a cone and exactly Euclidean outside of it. We achieve optimal shielding in the sense that the metric and extrinsic curvature { are controlled at a super-harmonic rate, regardless of how slowly they decay (even} beyond the standard ADM formalism), and the gluing domain can be a collection of arbitrarily narrow nested cones. We also uncover several notions of independent interest: silhouette functions, localized ADM modulator, and relative energy-momentum vector. An axisymmetric example is provided numerically.
format Preprint
id arxiv_https___arxiv_org_abs_2402_17598
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Optimal shielding for Einstein gravity
Floch, Bruno Le
LeFloch, Philippe G.
General Relativity and Quantum Cosmology
Analysis of PDEs
To construct asymptotically-Euclidean Einstein's initial data sets, we introduce the localized seed-to-solution method, which projects from approximate to exact solutions of the Einstein constraints. The method enables us to glue together initial data sets in multiple asymptotically-conical regions, and in particular construct data sets that exhibit the gravity shielding phenomenon, specifically that are localized in a cone and exactly Euclidean outside of it. We achieve optimal shielding in the sense that the metric and extrinsic curvature { are controlled at a super-harmonic rate, regardless of how slowly they decay (even} beyond the standard ADM formalism), and the gluing domain can be a collection of arbitrarily narrow nested cones. We also uncover several notions of independent interest: silhouette functions, localized ADM modulator, and relative energy-momentum vector. An axisymmetric example is provided numerically.
title Optimal shielding for Einstein gravity
topic General Relativity and Quantum Cosmology
Analysis of PDEs
url https://arxiv.org/abs/2402.17598