We present new results from two codes, using finite differencing and pseudo-spectral methods for the wave equations in (3+1) dimensions. We use a hyperboloidal transformation which allows direct access to null infinity and simplifies the control over characteristic speeds on Kerr-Schild backgrounds. We show that this method is ideal for attaching hyperboloidal slices or for adapting the numerical resolution in certain spacetime regions. As an example application, we study late-time Kerr tails of sub-dominant modes and obtain new insight into the splitting of decay rates. The involved conformal wave equation is freed of formally singular terms whose numerical evaluation might be problematically close to future null infinity
We use rigorous techniques from numerical analysis of hyperbolic equations in bounded domains to con...
International audienceWe study quasinormal modes of black holes, with a focus on resonant (or quasin...
Numerical simulations of Kerr black holes are presented and the excitation of quasinormal modes is s...
We present new results from two codes, using finite differencing and pseudo-spectral methods for the...
We describe the hyperboloidal compactification for Teukolsky equations in Kerr spacetime. We include...
We analyze stationary slicings of the Schwarzschild spacetime defined by members of the Bona-Masso f...
Abstract. The numerical investigation of wave propagation in the asymptotic domain of Kerr spacetime...
We discuss the hyperboloidal evolution problem in general relativity from a numerical perspective, a...
We study gravitational perturbations of Schwarzschild spacetime by solving a hyperboloidal initial v...
Abstract. We construct initial data corresponding to a single perturbed Kerr black hole in vacuum. T...
We construct quasimodes for the Klein–Gordon equation on the black hole exterior of Kerr–AdS (anti- ...
We discuss a gauge choice which allows us to avoid the introduction of artificial timelike outer bou...
We consider an approach to the hyperboloidal evolution problem based on the Einstein equations writt...
The hyperboloidal initial value problem is addressed in the context of Numerical Relativity, motivat...
With the example of the spherically symmetric scalar wave equation on Minkowski space-time we demons...
We use rigorous techniques from numerical analysis of hyperbolic equations in bounded domains to con...
International audienceWe study quasinormal modes of black holes, with a focus on resonant (or quasin...
Numerical simulations of Kerr black holes are presented and the excitation of quasinormal modes is s...
We present new results from two codes, using finite differencing and pseudo-spectral methods for the...
We describe the hyperboloidal compactification for Teukolsky equations in Kerr spacetime. We include...
We analyze stationary slicings of the Schwarzschild spacetime defined by members of the Bona-Masso f...
Abstract. The numerical investigation of wave propagation in the asymptotic domain of Kerr spacetime...
We discuss the hyperboloidal evolution problem in general relativity from a numerical perspective, a...
We study gravitational perturbations of Schwarzschild spacetime by solving a hyperboloidal initial v...
Abstract. We construct initial data corresponding to a single perturbed Kerr black hole in vacuum. T...
We construct quasimodes for the Klein–Gordon equation on the black hole exterior of Kerr–AdS (anti- ...
We discuss a gauge choice which allows us to avoid the introduction of artificial timelike outer bou...
We consider an approach to the hyperboloidal evolution problem based on the Einstein equations writt...
The hyperboloidal initial value problem is addressed in the context of Numerical Relativity, motivat...
With the example of the spherically symmetric scalar wave equation on Minkowski space-time we demons...
We use rigorous techniques from numerical analysis of hyperbolic equations in bounded domains to con...
International audienceWe study quasinormal modes of black holes, with a focus on resonant (or quasin...
Numerical simulations of Kerr black holes are presented and the excitation of quasinormal modes is s...