Boosted three-dimensional black-hole evolutions with singularity excision
The Binary Black Hole Grand Challenge Alliance: G. B. Cook, M. F. Huq,, S. A. Klasky, M. A. Scheel, A. M. Abrahams, A. Anderson, P. Anninos, T. W., Baumgarte, N. T. Bishop, S. R. Brandt, J. C. Browne, K. Camarda, M. W., Choptuik, C. R. Evans, L. S. Finn, G. C. Fox, R. Gomez

TL;DR
This paper demonstrates a successful 3D numerical evolution of a moving black hole using Cauchy methods, advancing the modeling of binary black hole interactions and gravitational wave predictions.
Contribution
It introduces a novel 3D black hole evolution technique with singularity excision, including the first free-moving black hole simulation in this framework.
Findings
First successful simulation of a moving black hole in 3D
Black hole moved ~6M at 0.1c during ~60M evolution
Advances toward modeling binary black hole interactions
Abstract
Binary 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 ~6M at 0.1c during a total evolution of duration ~60M.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
