Publication date
January 2016
DOIAbstract
It is proven that for smooth initial data with compact support outside the event horizon, the solution of every azimuthal mode of the Teukolsky equation for general spin decays pointwise in time
It is proven that for smooth initial data with compact support outside the event horizon, the solution of every azimuthal mode of the Teukolsky equation for general spin decays pointwise in time
We present a generalization of previous results regarding the stability under gravitational perturba...
We present a generalization of previous results regarding the stability under gravitational perturba...
We uncover hidden spectral symmetries of the Teukolsky equation in Kerr(-de Sitter) black holes, rec...
It is proven that for smooth initial data with compact support outside the event horizon, the soluti...
It is proven that for smooth initial data with compact support outside the event horizon, the soluti...
It is proven that for smooth initial data with compact support outside the event horizon, the soluti...
After a brief introduction to the black hole stability problem, we outline our recent proof of the l...
After a brief introduction to the black hole stability problem, we outline our recent proof of the l...
After a brief introduction to the black hole stability problem, we outline our recent proof of the l...
Abstract: We prove that there are no exponentially growing modes nor modes on the real axis for the ...
We prove that the Schwarzschild black hole is linearly stable under electromagnetic and gravitationa...
We prove that the Schwarzschild black hole is linearly stable under electromagnetic and gravitationa...
We prove that the Schwarzschild black hole is linearly stable under electromagnetic and gravitationa...
Abstract: We prove that there are no exponentially growing modes nor modes on the real axis for the ...
In this paper we consider the possible existence of unstable axisymmetric modes in Kerr space times,...
We present a generalization of previous results regarding the stability under gravitational perturba...
We present a generalization of previous results regarding the stability under gravitational perturba...
We uncover hidden spectral symmetries of the Teukolsky equation in Kerr(-de Sitter) black holes, rec...
It is proven that for smooth initial data with compact support outside the event horizon, the soluti...
It is proven that for smooth initial data with compact support outside the event horizon, the soluti...
It is proven that for smooth initial data with compact support outside the event horizon, the soluti...
After a brief introduction to the black hole stability problem, we outline our recent proof of the l...
After a brief introduction to the black hole stability problem, we outline our recent proof of the l...
After a brief introduction to the black hole stability problem, we outline our recent proof of the l...
Abstract: We prove that there are no exponentially growing modes nor modes on the real axis for the ...
We prove that the Schwarzschild black hole is linearly stable under electromagnetic and gravitationa...
We prove that the Schwarzschild black hole is linearly stable under electromagnetic and gravitationa...
We prove that the Schwarzschild black hole is linearly stable under electromagnetic and gravitationa...
Abstract: We prove that there are no exponentially growing modes nor modes on the real axis for the ...
In this paper we consider the possible existence of unstable axisymmetric modes in Kerr space times,...
We present a generalization of previous results regarding the stability under gravitational perturba...
We present a generalization of previous results regarding the stability under gravitational perturba...
We uncover hidden spectral symmetries of the Teukolsky equation in Kerr(-de Sitter) black holes, rec...
Add to ORKG