2 papers
gr-qc1995
Simulations of Nonaxisymmetric Instability in a Rotating Star: A Comparison Between Eulerian and Smooth Particle Hydrodynamics
Scott C. Smith, Janet L. Houser, Joan M. Centrella
We have carried out 3-D numerical simulations of the dynamical bar instability in a rotating star and the resulting gravitational radiation using both an Eulerian code written in c…
gr-qc1994
A Three-Dimensional Hydrodynamics Code for Modeling Sources of Gravitational Radiation
Scott C. Smith, Joan M. Centrella, Sean P. Clancy
We have developed a 3-D Eulerian hydrodynamics code to model sources of gravitational radiation. The code is written in cylindrical coordinates and has moving grids…