We discuss the use of Adaptative Mesh Refinement (AMR) techniques in dynamical black hole spacetimes. We compare results between traditional fixed grid methods and a new AMR application for the 1-D Schwarzschild case.
Cite
@article{arxiv.gr-qc/9412057,
title = {Adaptative Mesh Refinement in Numerical Relativity},
author = {Joan Masso and Edward Seidel and Paul Walker},
journal= {arXiv preprint arXiv:gr-qc/9412057},
year = {2007}
}
Comments
3 pages, uuencoded gziped ps file including 2 Figs. Also available at http://jean-luc.ncsa.uiuc.edu/Papers/ To appear in the MG7 proceedings