演講資訊

摘要：

Core-collapse supernovae, which came from stellar explosions of very massive stars at the end of their lifetime, are expected to be a significant science target of gravitational wave detectors and high energy MeV neutrino detectors. In addition to observations of its electromagnetism emissions, combing observation data with its gravitational wave or neutrino signals enables us to comprehensively explore the underlying physics from a single source associated with different physical processes. In this talk, I would like to highlight the recent theoretical developments of core-collapse supernovae as multimessenger sources.