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次极端和极端雷斯纳 - 诺德斯特龙黑洞上无质量弗拉索夫方程的衰减与非衰减

Decay and non-decay for the massless Vlasov equation on subextremal and extremal Reissner-Nordström black holes.

作者信息

Weissenbacher Max

机构信息

Department of Mathematics, Imperial College London, South Kensington Campus, London, SW7 2AZ UK.

出版信息

Arch Ration Mech Anal. 2024;248(6):118. doi: 10.1007/s00205-024-02060-1. Epub 2024 Nov 20.

DOI:10.1007/s00205-024-02060-1
PMID:39582737
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC11579134/
Abstract

We study the massless Vlasov equation on the exterior of the subextremal and extremal Reissner-Nordström spacetimes. We prove that moments decay at an exponential rate in the subextremal case and at a polynomial rate in the extremal case. This polynomial rate is shown to be sharp along the event horizon. In the extremal case we show that transversal derivatives of certain components of the energy momentum tensor do not decay along the event horizon if the solution and its first time derivative are initially supported on a neighbourhood of the event horizon. The non-decay of transversal derivatives in the extremal case is compared to the work of Aretakis on instability for the wave equation. Unlike Aretakis' results for the wave equation, which exploit a hierarchy of conservation laws, our proof is based entirely on a quantitative analysis of the geodesic flow and conservation laws do not feature in the present work.

摘要

我们研究了次极端和极端雷斯纳 - 诺德斯特龙时空外部的无质量弗拉索夫方程。我们证明,在次极端情况下矩以指数速率衰减,而在极端情况下以多项式速率衰减。沿着事件视界,这种多项式速率被证明是精确的。在极端情况下,我们表明,如果解及其一阶时间导数最初在事件视界的一个邻域内有支撑,那么能量动量张量某些分量的横向导数沿事件视界不会衰减。将极端情况下横向导数的不衰减与阿雷塔基斯关于波动方程不稳定性的工作进行了比较。与阿雷塔基斯关于波动方程的结果不同,后者利用了守恒律的层次结构,我们的证明完全基于测地线流的定量分析,并且守恒律在本工作中没有出现。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c964/11579134/6b1a669a06a7/205_2024_2060_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c964/11579134/227931c09fb8/205_2024_2060_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c964/11579134/b755c2dfd5ed/205_2024_2060_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c964/11579134/6b1a669a06a7/205_2024_2060_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c964/11579134/227931c09fb8/205_2024_2060_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c964/11579134/b755c2dfd5ed/205_2024_2060_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/c964/11579134/6b1a669a06a7/205_2024_2060_Fig3_HTML.jpg

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本文引用的文献

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Asymptotic Stability of Minkowski Space-Time with Non-compactly Supported Massless Vlasov Matter.具有非紧支无质量弗拉索夫物质的闵可夫斯基时空的渐近稳定性
Arch Ration Mech Anal. 2021;242(1):1-147. doi: 10.1007/s00205-021-01639-2. Epub 2021 Jul 22.
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A Non-degenerate Scattering Theory for the Wave Equation on Extremal Reissner-Nordström.关于极端雷斯纳 - 诺德斯特龙时空波动方程的非简并散射理论
Commun Math Phys. 2020;380(1):323-408. doi: 10.1007/s00220-020-03857-3. Epub 2020 Sep 23.
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