Stable characteristic evolution of generic 3-dimensional single-black-hole spacetimes
General Relativity and Quantum Cosmology
2012-08-27 v1
Abstract
We report new results which establish that the accurate 3-dimensional numerical simulation of generic single-black-hole spacetimes has been achieved by characteristic evolution with unlimited long term stability. Our results cover a selection of distorted, moving and spinning single black holes, with evolution times up to 60,000M.
Cite
@article{arxiv.gr-qc/9801069,
title = {Stable characteristic evolution of generic 3-dimensional single-black-hole spacetimes},
author = {The Binary Black Hole Grand Challenge Alliance and : and R. Gomez and L. Lehner and R. Marsa and J. Winicour and A. Abrahams and A. Anderson and P. Anninos and T. Baumgarte and N. Bishop and S. Brandt J. Browne and K. Camarda and M. Choptuik and R. Correl and G. Cook and C. Evans and L. Finn and G. Fox and T. Haupt and M. Huq and L. Kidder and S. Klasky and P. Laguna and W. Landry and J. Lenaghan and J. Masso and R. A. Matzner and S. Mitra and P. Papadopoulos and M. Parashar and L. Rezzolla and M. Rupright and F. Saied and P. Saylor and M. Scheel and E. Seidel and S. Shapiro and D. Shoemaker and L. Smarr and B. Szilagyi and A. Teukolsky and M. H. P. M. van Putten and P. Walker and J. W. York},
journal= {arXiv preprint arXiv:gr-qc/9801069},
year = {2012}
}
Comments
4 pages, 3 figures