12/12 Multi-messenger signals from magnetized core-collapse supernovae
Time: 1:20pm~3:10pm, December 12 (Thursday)
Title: Multi-messenger signals from magnetized core-collapse supernovae
Speaker: Associate Professor Kuo-Chuan Pan
(Institute of Astronomy, National Tsing Hua University)
Place: Science Building III SC157
Abstract:
Core-collapse supernovae (CCSNe) are among the most explosive events in the universe and are the birthplaces of neutron stars and stellar-mass black holes under extreme conditions. CCSNe are also ideal multi-messenger sources, expected to be detected not only through electromagnetic waves but also via neutrinos and gravitational waves.
In this talk, I will present the latest results from our multi-dimensional supernova simulations with self-consistent neutrino transport. In particular, I will focus on how magnetic fields and stellar rotation affect the explosion engine and multi-messenger signals. I will also comment on further searches for gravitational waves from core-collapse supernovae.