Structure of stable binary neutron star merger remnants: Role of initial spinW. Kastaun, Bruno Giacomazzo|Physical review. D/Physical review. D.|2017Cited by 60
Robust recovery of primitive variables in relativistic ideal magnetohydrodynamicsW. Kastaun, R. Ciolfi|Physical review. D/Physical review. D.|2021Cited by 51
Numerical inside view of hypermassive remnant models for GW170817W. Kastaun, F. Ohme|Physical review. D/Physical review. D.|2021Cited by 13