Library to create initial data for rotating neutron stars using Stergioulas' RNS code and import them to Cartesian grids for 3+1 evolutions.
The original code is based on the method developed by Komatsu, Eriguchi & Hachisu (1989) and modifications introduced by Cook, Shapiro & Teukolsky (1994) and detailed in Stergioulas and Friedman (1995) and Nozawa, Stergioulas, Gourgoulhon & Eriguchi (1998).
This code is a stand-alone, early version of the Cactus/WhiskyRNSID module by SB, that ultimately finished in the Cactus/Einstein Toolkit.
See Issues for known issues and possible improvements.
HISTORY
- SB 07/2022 started