most citedA new numerical scheme to compute 3D configurations of quasiequilibrium compact stars in general relativity -- Application to synchronously rotating binary star systems --

22 citations · 22 across the 1 of their papers we have counts for

collaborators

1 paper

gr-qc1999★ 22 cited

A new numerical scheme to compute 3D configurations of quasiequilibrium compact stars in general relativity -- Application to synchronously rotating binary star systems --

Fumihiko Usui, Koji Uryu, Yoshiharu Eriguchi

We have developed a new numerical scheme to obtain quasiequilibrium structures of nonaxisymmetric compact stars such as binary neutron star systems as well as the spacetime around…