Physics of Core-Collapse Supernovae and Compact Star Formations
Aim of Workshop
The aim of this workshop is to gather the latest knowledge on both macro- and microphysics of relevance for core-collapse supernova explosions and ensuing compact-star formations. It has been already some time since spatially 3-dimensional supernova simulations became feasible and these days numerical schemes are getting more sophisticated and microphysics incorporated in simulations are being scrutinized. In the wake of the first detection of a neutron star merger via gravitational waves, on the other hand, interest in the equation of state of hot and dense hadronic matter is very high. In this workshop we invite leading researchers on the topics listed below and discuss the latest issues in a broad context of compact-star formations.
Topics
EOS of hot and dense hadronic matter relevant for core-collapse supernovae and proto neutron stars
Supernova simulations with multi-dimensional neutrino transport
Weak interactions and neutrino emissions in core-collapse supernovae and proto neutron star cooling
Neutrino oscillations in core-collapse supernova cores and proto neutron stars
Neutron star mergers: gravitational waves, EOS and nucleosynthesis
Invited speakers
Atsushi Tamii (Osaka univ.)
David Radice (Princeton univ.)
Hong Shen (Nankai univ.)
Jinniu Hu (Nankai univ.)
Jonas Lippuner (LANL)
Kohsuke Sumiyoshi (NCT)
Luca Baiotti (Osaka univ.)
Luke Roberts (Michigan State univ.)
Oliver Just (RIKEN)
Remco Zegers (NSCL)
Stefan Typel (GSI)
Volpe Maria Cristina (ACP)
Yuichiro Sekiguchi (Toho univ.)
Important dates
The deadline for contribution talks and travel supports: 19, February, 2018
The deadline for poster presentations and only admission (including banquet): 28, February, 2018