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 derive the Teukolsky equation for perturbations of a Kerr spacetime when the spacetime metric is ...
Abstract: The reduced (in the angular coordinate ϕ) wave equation and Klein–Gordon equation are cons...
International audienceWe study the peeling on Kerr spacetime for fields satisfying conformally invar...
We present new results from two codes, using finite differencing and pseudo-spectral methods for the...
Abstract. The numerical investigation of wave propagation in the asymptotic domain of Kerr spacetime...
We describe the hyperboloidal compactification for Teukolsky equations in Kerr spacetime. We include...
We discuss the hyperboloidal evolution problem in general relativity from a numerical perspective, a...
Abstract. We construct initial data corresponding to a single perturbed Kerr black hole in vacuum. T...
International audienceWe study quasinormal modes of black holes, with a focus on resonant (or quasin...
The hyperboloidal initial value problem is addressed in the context of Numerical Relativity, motivat...
We study gravitational perturbations of Schwarzschild spacetime by solving a hyperboloidal initial v...
We consider an approach to the hyperboloidal evolution problem based on the Einstein equations writt...
We show how to solve hyperbolic equations numerically on unbounded domains by compactification, ther...
We analyze stationary slicings of the Schwarzschild spacetime defined by members of the Bona–Massó f...
In this bachelor thesis we discuss the effects of compactification and hyperboloidal slicing of spac...
We derive the Teukolsky equation for perturbations of a Kerr spacetime when the spacetime metric is ...
Abstract: The reduced (in the angular coordinate ϕ) wave equation and Klein–Gordon equation are cons...
International audienceWe study the peeling on Kerr spacetime for fields satisfying conformally invar...
We present new results from two codes, using finite differencing and pseudo-spectral methods for the...
Abstract. The numerical investigation of wave propagation in the asymptotic domain of Kerr spacetime...
We describe the hyperboloidal compactification for Teukolsky equations in Kerr spacetime. We include...
We discuss the hyperboloidal evolution problem in general relativity from a numerical perspective, a...
Abstract. We construct initial data corresponding to a single perturbed Kerr black hole in vacuum. T...
International audienceWe study quasinormal modes of black holes, with a focus on resonant (or quasin...
The hyperboloidal initial value problem is addressed in the context of Numerical Relativity, motivat...
We study gravitational perturbations of Schwarzschild spacetime by solving a hyperboloidal initial v...
We consider an approach to the hyperboloidal evolution problem based on the Einstein equations writt...
We show how to solve hyperbolic equations numerically on unbounded domains by compactification, ther...
We analyze stationary slicings of the Schwarzschild spacetime defined by members of the Bona–Massó f...
In this bachelor thesis we discuss the effects of compactification and hyperboloidal slicing of spac...
We derive the Teukolsky equation for perturbations of a Kerr spacetime when the spacetime metric is ...
Abstract: The reduced (in the angular coordinate ϕ) wave equation and Klein–Gordon equation are cons...
International audienceWe study the peeling on Kerr spacetime for fields satisfying conformally invar...