Orateur
Dr
Kei Kotake
(Fukuoka University)
Description
Based on our 3D(-GR) simulations with spectral (or gray) neutrino
transport using non-rotating and rapidly rotating progenitors,
we report the gravitational-wave (GW) signatures and discuss the
detectability in both 2nd and 3rd generation interferometers.
We also discuss how we can extract information of the central engine
based on detailed correlation analysis of the GW and neutrino signals.
Auteur principal
Dr
Kei Kotake
(Fukuoka University)
