Turnitin
降AI改写
早检测系统
早降重系统
Turnitin-UK版
万方检测-期刊版
维普编辑部版
Grammarly检测
Paperpass检测
checkpass检测
PaperYY检测
The global non-linear stability of the Kerr–de Sitter family of black holes
We establish the full global non-linear stability of the Kerr–de Sitter family of black holes, as
solutions of the initial value problem for the Einstein vacuum equations with positive …
solutions of the initial value problem for the Einstein vacuum equations with positive …
Quantum instability of the Cauchy horizon in Reissner–Nordström–deSitter spacetime
S Hollands, RM Wald, J Zahn - Classical and Quantum Gravity, 2020 - iopscience.iop.org
In classical general relativity, the values of fields on spacetime are uniquely determined by
their values at an initial time within the domain of dependence of this initial data surface …
their values at an initial time within the domain of dependence of this initial data surface …
A sharp version of Price's law for wave decay on asymptotically flat spacetimes
We prove Price's law with an explicit leading order term for solutions ϕ (t, x) of the scalar
wave equation on a class of stationary asymptotically flat (3+ 1)-dimensional spacetimes …
wave equation on a class of stationary asymptotically flat (3+ 1)-dimensional spacetimes …
Strong cosmic censorship in charged black-hole spacetimes: still subtle
It was recently shown that strong cosmic censorship may be violated in highly charged black-
hole spacetimes living in a universe with a positive cosmological constant. Several follow-up …
hole spacetimes living in a universe with a positive cosmological constant. Several follow-up …
Linear stability of slowly rotating Kerr black holes
We prove the linear stability of slowly rotating Kerr black holes as solutions of the Einstein
vacuum equations: linearized perturbations of a Kerr metric decay at an inverse polynomial …
vacuum equations: linearized perturbations of a Kerr metric decay at an inverse polynomial …
Mathematical study of scattering resonances
Mathematical study of scattering resonances | Bulletin of Mathematical Sciences Skip to main
content SpringerLink Account Menu Find a journal Publish with us Track your research Search …
content SpringerLink Account Menu Find a journal Publish with us Track your research Search …
[HTML][HTML] Analysis of linear waves near the Cauchy horizon of cosmological black holes
We show that linear scalar waves are bounded and continuous up to the Cauchy horizon of
Reissner–Nordström–de Sitter and Kerr–de Sitter spacetimes and in fact decay …
Reissner–Nordström–de Sitter and Kerr–de Sitter spacetimes and in fact decay …
Optimal decay for solutions of the Teukolsky equation on the Kerr metric for the full subextremal range| a|< M
P Millet - arxiv preprint arxiv:2302.06946, 2023 - arxiv.org
We derive the large time asymptotics of initially regular and localized solutions of the
Teukolsky equation on the exterior of a subextremal Kerr black hole for any half integer spin …
Teukolsky equation on the exterior of a subextremal Kerr black hole for any half integer spin …
Non-linear stability of the Kerr–Newman–de Sitter family of charged black holes
We prove the global non-linear stability, without symmetry assumptions, of slowly rotating
charged black holes in de Sitter spacetimes in the context of the initial value problem for the …
charged black holes in de Sitter spacetimes in the context of the initial value problem for the …
Mode stability and shallow quasinormal modes of Kerr–de Sitter black holes away from extremality
A Kerr–de Sitter black hole is a solution. M; gƒ; m; a/of the Einstein vacuum equations with
cosmological constant ƒ> 0. It describes a black hole with mass m> 0 and specific angular …
cosmological constant ƒ> 0. It describes a black hole with mass m> 0 and specific angular …