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We analytically study the linear response of a near-extremal Kerr black hole to external scalar, electromagnetic, and gravitational field perturbations. We show that the energy density, electromagnetic field strength, and tidal force…

广义相对论与量子宇宙学 · 物理学 2016-10-19 Samuel E. Gralla , Aaron Zimmerman , Peter Zimmerman

In gravitational collapse leading to black hole formation, trapping horizons typically develop inside the contracting matter. Classically, an ingoing trapping horizon moves towards the centre where it reaches a curvature singularity, while…

广义相对论与量子宇宙学 · 物理学 2018-10-03 Pierre Binétruy , Alexis Helou , Frédéric Lamy

Persistent puzzles to do with information loss for black holes have stimulated critical reassessment of the domain of validity of semiclassical EFT reasoning in curved spacetimes, particularly in the presence of horizons. We argue here that…

高能物理 - 理论 · 物理学 2020-03-04 C. P. Burgess , Joshua Hainge , Greg Kaplanek , Markus Rummel

Massive spin-2 fields, which arise in proposed extensions of the standard model of particle physics and general relativity, give rise to a superradiant instability around spinning black holes. We study the nonlinear evolution of this…

广义相对论与量子宇宙学 · 物理学 2025-09-18 Taillte May , William E. East

Extreme black holes have been argued to be unstable, in the sense that under linearized gravitational perturbations of the extreme Kerr spacetime the Weyl scalar $\psi_4$ blows up along their event horizons at very late advanced times. We…

广义相对论与量子宇宙学 · 物理学 2018-04-04 Lior M. Burko , Gaurav Khanna

A naive introduction of a dependency of the mass of a black hole on the Schwarzschild time coordinate results in singular behavior of curvature invariants at the horizon, violating expectations from complementarity. If instead a temporal…

广义相对论与量子宇宙学 · 物理学 2008-11-26 James Lindesay

We investigate new paths to black hole formation by considering the general relativistic evolution of a differentially rotating polytrope with toroidal shape. We find that this polytrope is unstable to nonaxisymmetric modes, which leads to…

广义相对论与量子宇宙学 · 物理学 2010-11-16 Burkhard Zink , Nikolaos Stergioulas , Ian Hawke , Christian D. Ott , Erik Schnetter , Ewald Mueller

The non-linear generation of harmonics in gravitational perturbations of black holes is explored using numerical relativity based on an in-going light-cone framework. Localised, finite, perturbations of an isolated black hole are…

广义相对论与量子宇宙学 · 物理学 2009-11-07 Philippos Papadopoulos

Extremal planar black holes of four dimensional Einstein-Maxwell theory with a negative cosmological constant have an AdS$_2 \times \R^2$ near horizon geometry. We show that this near horizon geometry admits a deformation to a two parameter…

高能物理 - 理论 · 物理学 2015-06-19 Sean A. Hartnoll , Jorge E. Santos

We show that extremal Kerr black holes are sensitive probes of new physics. Stringy or quantum corrections to general relativity are expected to generate higher-curvature terms in the gravitational action. We show that in the presence of…

高能物理 - 理论 · 物理学 2024-07-11 Gary T. Horowitz , Maciej Kolanowski , Grant N. Remmen , Jorge E. Santos

We show that the general charged, rotating black hole in five-dimensional Einstein-Maxwell theory has a singular extremal limit. Only the known analytic solutions with exactly zero charge or zero angular momenta have smooth extremal…

高能物理 - 理论 · 物理学 2024-12-11 Gary T. Horowitz , Jorge E. Santos

We prove a new type of finite time blow-up for a class of semilinear wave equations on extremal black holes. The initial data can be taken to be arbitrarily close to the trivial data. The first singularity occurs along the (degenerate)…

广义相对论与量子宇宙学 · 物理学 2015-06-15 Stefanos Aretakis

Spacetimes with an ergoregion that is not connected to a horizon are linearly unstable. While the linear regime has been studied in a number of settings, little is known about the nonlinear evolution of this ergoregion instability. Here, we…

广义相对论与量子宇宙学 · 物理学 2025-12-12 Nils Siemonsen , William E. East

Black holes display universal behavior near extremality. One such feature is the late-time blowup of derivatives of linearized perturbations across the horizon. For generic initial data, this instability is regulated by backreaction, and…

高能物理 - 理论 · 物理学 2019-02-20 Shahar Hadar

For a stationary and axisymmetric black hole, there is a natural way to split the fields into a probe sector and a background sector. The equations of motion for the probe sector enjoy a significantly enhanced symmetry on the black hole…

高能物理 - 理论 · 物理学 2014-04-23 Jianwei Mei

We investigate the generic behaviour of marginally trapped tubes (roughly time-evolved apparent horizons) using simple, spherically symmetric examples of dust and scalar field collapse/accretion onto pre-existing black holes. We find that…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Ivan Booth , Lionel Brits , Jose A. Gonzalez , Chris Van Den Broeck

The Cauchy horizon inside a perturbed Kerr black hole develops an instability that transforms it into a curvature singularity. We solve for the linearized Weyl scalars $\psi_0$ and $\psi_4$ and for the curvature scalar…

广义相对论与量子宇宙学 · 物理学 2017-12-05 Lior M. Burko , Gaurav Khanna , Anıl Zenginoǧlu

Singular solutions of the harmonic Einstein evolution equation are constructed which are related to spatially global and time-local solutions for a certain class of quasilinear hyperbolic systems of second order. The constructed…

偏微分方程分析 · 数学 2016-03-30 Joerg Kampen

Recently, much attention has been focused on the false vacuum islands that are flooded by an expanding ocean of true-vacuum bubbles slightly later than most of the other parts of the world. These delayed decay regions will accumulate…

宇宙学与河外天体物理 · 物理学 2024-08-06 Rong-Gen Cai , Yu-Shi Hao , Shao-Jiang Wang

It has recently been argued that extremal black holes can act as amplifiers of new physics, due to horizon instabilities that enhance the effects of ultraviolet corrections. In this paper, we revisit some of these claims and investigate the…

广义相对论与量子宇宙学 · 物理学 2026-02-05 Francesco Di Filippo , Shinji Mukohyama , José M. M. Senovilla