超新星爆発からのマルチメッセンジャー
研究会について
- 日時：
- 2013年12月2日（月）～6日（金）
- 場所：
- 福岡大学 理学部物理科学科
- 共催：
- 基盤研究「次世代計算機・観測から迫る高エネルギー爆発天体現象の理論的解明」
基盤研究「中心エンジンから解き明かすガンマ線バースト放射機構」
基盤研究「大質量星の進化における重力崩壊型超新星の総合的研究」
HPCI戦略プログラム分野5「物質と宇宙の起源と構造」 - web：
- http://www.cis.fukuoka-u.ac.jp/~kkotake/sn_MM13.html
Aims of the Workshop
The aim of the workshop is to set an opportunity for specialists around the world who are now touching to 3D, general relativistic, Boltzmann neutrino transport to meet together and have exciting discussions with world-leading observers (including KAGRA, Super-Kamiokande, Subaru, Suzaku, etc) and their data-analyst on the SN multi-messengers produced deep inside the central core.
Such an exciting encounter that is intended to bridge theory and observation, will provide wonderful opportunities to start a future collaboration, only by which a great progress will be brought about on our understanding of time-honored puzzles about supernova mechanisms.
Topics
– Explosion theory of core-collapse supernovae
– How to detect neutrinos and gravitational waves from next nearby supernova event and what we can learn from them ?
– Nucleosynthesis
– Strategy toward multi-messenger astronomy of compact objects
– Roles of magnetic fields
– Weak interactions and equations of state for dense matter
– Supernova Remnants
– Efficient supercomputing algorithms for stellar core-collapse simulations
Tentative Invited Speakers (* to be confirmed)
M. Ando (U Tokyo)
S. Couch (U Chicago)
K. Hayama (Osaka-city U)
S. Horiuchi (UCI)
S. Katsuda (RIKEN)
J. Kneller (NC state)
Y. Koshio (U Okayama)
Y. Masada (U Kobe)
B. Messer (ORNL)
K. Nakazato (TUS)
M. Obergaulinger (U Valencia)
C. Ott (Caltech)
G. Shen (TU Darmstadt)
T. Takiwaki (NAOJ)
M. Tanaka (NAOJ)
M. Vagins (IPMU)
S. Wanajo (NAOJ)
S. Yamada (Waseda U)
Scientific Organizers
K. Sato (NINS), S. Yamada (Waseda U), Kohsuke Sumiyoshi (Numazu College),Tomoya Takiwaki (NAOJ),Yudai Suwa (YITP), Takami Kuroda (Basel U),Kei Kotake (Fukuoka U: co-ordinator)
Contact
kkotake [at] fukuoka-u.ac.jp
