315 citations · 1.1k across the 35 of their papers we have counts for
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The linearized Einstein equations with sources
Peter Hintz
On vacuum spacetimes of general dimension, we study the linearized Einstein vacuum equations with a spatially compactly supported and (necessarily) divergence-free source. We prove…
Gluing small black holes along timelike geodesics I: formal solution
Peter Hintz
Given a smooth globally hyperbolic -dimensional spacetime satisfying the Einstein vacuum equations (possibly with cosmological constant) and an inextendible timelike geodesi…
Mode stability and shallow quasinormal modes of Kerr-de Sitter black holes away from extremality
Peter Hintz
A Kerr-de Sitter black hole is a solution of the Einstein vacuum equations with cosmological constant . It describes a black hole with ma…
Quasinormal modes of small Schwarzschild-de Sitter black holes
Peter Hintz, YuQing Xie
We study the behavior of the quasinormal modes (QNMs) of massless and massive linear waves on Schwarzschild-de Sitter black holes as the black hole mass tends to 0. Via uniform est…
Quasinormal modes and dual resonant states on de Sitter space
Peter Hintz, YuQing Xie
The existence of quasinormal modes (QNMs) for waves propagating on pure de Sitter space has been called into question in several works. We definitively prove the existence of quasi…
Strong cosmic censorship in charged black-hole spacetimes: still subtle
Vitor Cardoso, Joao L. Costa, Kyriakos Destounis +2
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 foll…
Quasinormal modes and Strong Cosmic Censorship
Vitor Cardoso, Joao L. Costa, Kyriakos Destounis +2
The fate of Cauchy horizons, such as those found inside charged black holes, is intrinsically connected to the decay of small perturbations exterior to the event horizon. As such,…
Uniqueness of Kerr-Newman-de Sitter black holes with small angular momenta
Peter Hintz
We show that a stationary solution of the Einstein-Maxwell equations which is close to a non-degenerate Reissner-Nordström-de Sitter solution is in fact equal to a slowly rotating…