Kasner Bounces and Fluctuating Collapse Inside Hairy Black Holes with Charged Matter

IF 2.4 1区 数学 Q1 MATHEMATICS Annals of Pde Pub Date : 2025-01-04 DOI:10.1007/s40818-024-00192-x
Warren Li, Maxime Van de Moortel
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Abstract

We study the interior of black holes in the presence of charged scalar hair of small amplitude \(\epsilon \) on the event horizon and show their terminal boundary is a crushing Kasner-like singularity. These spacetimes are spherically symmetric, spatially homogeneous and they differ significantly from the hairy black holes with uncharged matter previously studied in [M. Van de Moortel, Violent nonlinear collapse inside charged hairy black holes, Arch. Rational. Mech. Anal., 248, 89, 2024] in that the electric field is dynamical and subject to the backreaction of charged matter. We prove this charged backreaction causes drastically different dynamics compared to the uncharged case that ultimately impact the formation of the spacelike singularity, exhibiting novel phenomena such as

  • Collapsed oscillations: oscillatory growth of the scalar hair, nonlinearly induced by the collapse

  • A fluctuating collapse: The final Kasner exponents’ dependency in \(\epsilon \) is via an expression of the form

    \(|\sin \left( \omega _0 \cdot \epsilon ^{-2}+ O(\log (\epsilon ^{-1}))\right) |\).

  • A Kasner bounce: a transition from an unstable Kasner metric to a different stable Kasner metric

The Kasner bounce occurring in our spacetime is reminiscent of the celebrated BKL scenario in cosmology.

We additionally propose a construction indicating the relevance of the above phenomena – including Kasner bounces – to spacelike singularities inside more general (asymptotically flat) black holes, beyond the hairy case.

While our result applies to all values of \(\Lambda \in \mathbb {R}\), in the \(\Lambda <0\) case, our spacetime corresponds to the interior region of a charged asymptotically Anti-de-Sitter stationary black hole, also known as a holographic superconductor in high-energy physics, and whose exterior region was rigorously constructed in the recent mathematical work [W. Zheng, Asymptotically Anti-de Sitter Spherically Symmetric Hairy Black Holes, arXiv.2410.04758].

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带带电物质的毛状黑洞内的卡斯纳弹跳和波动坍缩
我们研究了视界上存在小振幅的带电标量毛发\(\epsilon \)的黑洞内部,并表明它们的终端边界是一个破碎的卡斯纳样奇点。这些时空是球对称的,空间均匀的,它们与以前在[M. M.]研究的带有不带电物质的毛状黑洞有很大的不同。Van de Moortel,带电毛状黑洞内的剧烈非线性坍缩,Arch。理性。械甲怪。分析的。[j], 248, 89, 2024],即电场是动态的,受带电物质的反作用影响。我们证明,与不带电的情况相比,这种带电的反反应导致了截然不同的动力学,最终影响了类空间奇点的形成,表现出新的现象,如塌缩振荡:标量毛发的振荡生长,非线性地由塌缩引起。最终Kasner指数在\(\epsilon \)中的依赖关系是通过\(|\sin \left( \omega _0 \cdot \epsilon ^{-2}+ O(\log (\epsilon ^{-1}))\right) |\)形式的表达式表示的。Kasner弹跳:从一个不稳定的Kasner度规到另一个稳定的Kasner度规的转变。Kasner弹跳发生在我们的时空中,让人想起宇宙学中著名的BKL场景。我们还提出了一个结构,表明上述现象(包括卡斯纳反弹)与更一般(渐近平坦)黑洞内的类空间奇点的相关性,超出了毛茸茸的情况。虽然我们的结果适用于\(\Lambda \in \mathbb {R}\)的所有值,但在\(\Lambda <0\)的情况下,我们的时空对应于带电渐近Anti-de-Sitter静止黑洞的内部区域,在高能物理中也称为全息超导体,其外部区域在最近的数学工作中被严格构建[W。郑,渐近反德西特球对称毛状黑洞,物理学报,vol . 39(10): 971 - 974。
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Annals of Pde
Annals of Pde Mathematics-Geometry and Topology
CiteScore
3.70
自引率
3.60%
发文量
22
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