Speaker
Kei Kotake
(Fukuoka University)
Description
Based on our three-dimensional hydrodynamic simulations of core-collapse supernovae (CCSN) including spectral neutrino transport, we present the gravitational-wave signatures emitted from a wide variety of SN progenitors. We also discuss how we can learn about the supernova mechanism by taking a correlation analysis between the gravitationa-wave and neutrino signatures particularly in the case of the next Galactic source.
Primary author
Kei Kotake
(Fukuoka University)
