Add to ORKGBinary black-hole interactions provide potentially the strongest source of gravitational radiation for detectors currently under development. We present some results from the Binary Black Hole Grand Challenge Alliance three-dimensional Cauchy evolution module. These constitute essential steps towards modeling such interactions and predicting gravitational radiation waveforms. We report on single black-hole evolutions and the first successful demonstration of a black hole moving freely through a three-dimensional computational grid via a Cauchy evolution: a hole moving near 6M at 0.1c during a total evolution of duration near 60M
The evolution of black holes in “confining boxes” is interesting for a number of reasons, particular...
The standard approach to the numerical evolution of black hole data using the ADM formulation with m...
We present a new many-parameter family of hyperbolic representations of Einstein’s equations, which ...
Binary black-hole interactions provide potentially the strongest source of gravitational radiation f...
Binary black hole interactions provide potentially the strongest source of gravitational radiation f...
We present the first fully relativistic longterm numerical evolutions of three equal-mass black hole...
We present the first simulations of non-headon (grazing) collisions of binary black holes in which t...
Initial data for two moving and spinning black holes in vacuum is constructed and evolved through a ...
We describe early success in the evolution of binary black-hole spacetimes with a numerical code bas...
We present the first fully relativistic longterm numerical evolutions of three equal-mass black hole...
We present new techniques for evolving binary black hole systems which allow the accurate determinat...
We present techniques for long-term, stable, and accurate evolutions of multiple-black-hole spacetim...
We present a new numerical code developed for the evolution of binary black-hole spacetimes using di...
We present the first simulations of non-headon (grazing) collisions of binary black holes in which t...
I review recent developments in numerical relativity, focussing on progress made in 3D black hole ev...
The evolution of black holes in “confining boxes” is interesting for a number of reasons, particular...
The standard approach to the numerical evolution of black hole data using the ADM formulation with m...
We present a new many-parameter family of hyperbolic representations of Einstein’s equations, which ...
Binary black-hole interactions provide potentially the strongest source of gravitational radiation f...
Binary black hole interactions provide potentially the strongest source of gravitational radiation f...
We present the first fully relativistic longterm numerical evolutions of three equal-mass black hole...
We present the first simulations of non-headon (grazing) collisions of binary black holes in which t...
Initial data for two moving and spinning black holes in vacuum is constructed and evolved through a ...
We describe early success in the evolution of binary black-hole spacetimes with a numerical code bas...
We present the first fully relativistic longterm numerical evolutions of three equal-mass black hole...
We present new techniques for evolving binary black hole systems which allow the accurate determinat...
We present techniques for long-term, stable, and accurate evolutions of multiple-black-hole spacetim...
We present a new numerical code developed for the evolution of binary black-hole spacetimes using di...
We present the first simulations of non-headon (grazing) collisions of binary black holes in which t...
I review recent developments in numerical relativity, focussing on progress made in 3D black hole ev...
The evolution of black holes in “confining boxes” is interesting for a number of reasons, particular...
The standard approach to the numerical evolution of black hole data using the ADM formulation with m...
We present a new many-parameter family of hyperbolic representations of Einstein’s equations, which ...