General Relativistic Numerical Simulations of Coalescing Binary Neutron Stars with Adaptive Mesh Refinement Methods
POSTER
Abstract
The poster reports the progress made in the construction of an adaptive mesh refinement enabled numerical code, GR-Astro, which enables such simulations, and its applications to the neutron star inspiral coalescences. Making use of the developments described above, we studied coalescing binary neutron star systems.