18-19 May 2015
神戸大学 瀧川記念学術交流会館
Japan timezone

超新星モデルの現状とニュートリノ信号

18 May 2015, 14:20
50m
大会議室 (神戸大学 瀧川記念学術交流会館)

大会議室

神戸大学 瀧川記念学術交流会館

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

Presentation Materials