Relativistic (3+1) Dimensional Hydrodynamic Simulations of Compact Interacting Binary Systems

摘要

We discuss the development of a relativistic hydrodynamic code for describing the evolution of astrophysical systems in three spatial dimensions. The application of this code to several test problems is presented. Preliminary results from the simulation of the dynamics of accreting binary white dwarf and neutron star systems are discussed. 14 refs., 4 figs. (ERA citation 12:010136)