Abstract
We report new results which establish that the accurate three-dimensional numerical simulation of generic single-black-hole spacetimes has been achieved by characteristic evolution with unlimited long term stability. Our results include distorted, moving, and spinning single black holes, with evolution times up to .
- Received 12 January 1998
DOI:https://doi.org/10.1103/PhysRevLett.80.3915
©1998 American Physical Society