We analyze stationary slicings of the Schwarzschild spacetime defined by members of the Bona–Massó family of slicing conditions. Our main focus is on the influence of a non-vanishing offset to the trace of the extrinsic curvature, which forbids the existence of standard Cauchy foliations but at the same time allows gauge choices that are adapted to include null infinity (\mathscr I) in the evolution. These hyperboloidal slicings are especially interesting for observing outgoing gravitational waves. We show that the standard 1+log slicing condition admits no overall regular hyperboloidal slicing, but by appropriately combining with harmonic slicing, we construct a gauge condition that leads to a strongly singularity-avoiding hyperboloidal fo...
Currently the most popular method to evolve black-hole binaries is the "moving puncture" method. It ...
We expand upon our previous analysis of numerical moving-puncture simulations of the Schwarzschild ...
We consider a family of spherical three-dimensional spacelike slices embedded in the Schwarzschild s...
We analyze stationary slicings of the Schwarzschild spacetime defined by members of the Bona–Massó f...
The hyperboloidal initial value problem is addressed in the context of Numerical Relativity, motivat...
We prove by explicit construction that there exists a maximal slicing of the Schwarzschild spacetime...
Slice stretching effects are discussed as they arise at the event horizon when geodesically slicing ...
We discuss the hyperboloidal evolution problem in general relativity from a numerical perspective, a...
International audienceWe study quasinormal modes of black holes, with a focus on resonant (or quasin...
We generalize Bowen-York black hole initial data to hyperboloidal constant mean curvature slices whi...
We study families of time-independent maximal and 1+log foliations of the Schwarzschild-Tangherlini ...
We review, without assuming symmetry, why time-independent endstates can be reached in black hole an...
We present new results from two codes, using finite differencing and pseudo-spectral methods for the...
Slice stretching effects such as slice sucking and slice wrapping arise when foliating the extended ...
There is constructed, for each member of a one-parameter family of cosmological models, which is obt...
Currently the most popular method to evolve black-hole binaries is the "moving puncture" method. It ...
We expand upon our previous analysis of numerical moving-puncture simulations of the Schwarzschild ...
We consider a family of spherical three-dimensional spacelike slices embedded in the Schwarzschild s...
We analyze stationary slicings of the Schwarzschild spacetime defined by members of the Bona–Massó f...
The hyperboloidal initial value problem is addressed in the context of Numerical Relativity, motivat...
We prove by explicit construction that there exists a maximal slicing of the Schwarzschild spacetime...
Slice stretching effects are discussed as they arise at the event horizon when geodesically slicing ...
We discuss the hyperboloidal evolution problem in general relativity from a numerical perspective, a...
International audienceWe study quasinormal modes of black holes, with a focus on resonant (or quasin...
We generalize Bowen-York black hole initial data to hyperboloidal constant mean curvature slices whi...
We study families of time-independent maximal and 1+log foliations of the Schwarzschild-Tangherlini ...
We review, without assuming symmetry, why time-independent endstates can be reached in black hole an...
We present new results from two codes, using finite differencing and pseudo-spectral methods for the...
Slice stretching effects such as slice sucking and slice wrapping arise when foliating the extended ...
There is constructed, for each member of a one-parameter family of cosmological models, which is obt...
Currently the most popular method to evolve black-hole binaries is the "moving puncture" method. It ...
We expand upon our previous analysis of numerical moving-puncture simulations of the Schwarzschild ...
We consider a family of spherical three-dimensional spacelike slices embedded in the Schwarzschild s...