Boosted three-dimensional black-hole evolutions with singularity excision
广义相对论与量子宇宙学
2012-08-27 v1
摘要
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.
引用
@article{arxiv.gr-qc/9711078,
title = {Boosted three-dimensional black-hole evolutions with singularity excision},
author = {The Binary Black Hole Grand Challenge Alliance and : and G. B. Cook and M. F. Huq and S. A. Klasky and M. A. Scheel and A. M. Abrahams and A. Anderson and P. Anninos and T. W. Baumgarte and N. T. Bishop and S. R. Brandt and J. C. Browne and K. Camarda and M. W. Choptuik and C. R. Evans and L. S. Finn and G. C. Fox and R. Gomez and T. Haupt and L. E. Kidder and P. Laguna and W. Landry and L. Lehner and J. Lenaghan and R. L. Marsa and J. Masso and R. A. Matzner and S. Mitra and P. Papadopoulos and M. Parashar and L. Rezzolla and M. E. Rupright and F. Saied and P. E. Saylor and E. Seidel and S. L. Shapiro and D. Shoemaker and L. Smarr and W. M. Suen and B. Szilagyi and S. A. Teukolsky and M. H. P. M. van Putten and P. Walker and J. Winicour and J. W. York},
journal= {arXiv preprint arXiv:gr-qc/9711078},
year = {2012}
}