Speaker
慶 固武
(福岡大)
Description
After we briefly review a current status of core-collapse supernova (CCSN) models and the neutrino and gravitational-wave predictions, we report our recent results about the CCSN observables based on our three-dimensional general relativistic simulations.
We will also discuss potential roles of the next generation detectors such as Hyper-Kamiokande and KAGRA to unravel the yet uncertain mechanism of explosion by deciphering the multi-messenger observables.
（参考文献）
reference: Simulations : http://ads.nao.ac.jp/abs/2012ApJ...755...11K
http://ads.nao.ac.jp/abs/2012PTEP.2012aA301K
GW signals : http://ads.nao.ac.jp/abs/2014PhRvD..89d4011K
http://ads.nao.ac.jp/abs/2013CRPhy..14..318K
Neutrino signals: in preperation
