Speaker
Dr
Kenta Kiuchi
(Max Planck Institute for Gravitational Physics)
Description
In this talk, I will present the recent progress of numerical modeling of compact binary mergers, which involves at least one neutron star in numerical relativity. Our group develops self-consistent modelings by performing a long-term numerical relativity neutrino-radiation magnetohydrodynamic simulation. I will present the details of the simulation results and perspective.
