Ponente
Descripción
Core collapse supernovae (CCSNe) mark the dramatic conclusion of massive stars' lives, serving as captivating laboratories for multi-messenger astrophysics, including neutrino and gravitational wave emissions, as well as the synthesis of heavy elements. Despite their significance, comprehending these events poses formidable challenges across theoretical, observational, and computational realms in astrophysics.
This seminar aims to provide an introductory exploration into the simulation of CCSNe, illustrating the key components of simulations and the prevailing challenges confronting the community. Furthermore, we will look into the observational implications of supernova simulations, giving insights into the alignment between theoretical models and empirical data, as well as observational constraints.
Moreover, the seminar will explore the detectability of core-collapse supernovae, focusing on the brief gravitational waves emitted during the collapse and the convective phases after it.
