GPPU Seminar
Modeling supernova neutrino emissions toward physics and multi-messenger astronomy in the next Galactic supernova
Yudai Suwa
(Univ. of Tokyo)
Date
15:00-17:00, July 26th, 2021Place
Zoom mapAbstract
天文学談話会 兼GPPUセミナー
Neutrinos are guaranteed observable from the next Galactic supernova (SN). Optical lights and gravitational waves are also observable but can be difficult to observe if SN location in the galaxy and the explosion details are unsuitable. The key to the next SN observation will be understanding various physical quantities using neutrinos first and then connecting them to other signals. In this seminar, I will discuss what physical quantities (e.g., mass and radius of neutron stars) can be extracted from observations using large statistical neutrinos as physics probes, and how to use these extracted physical quantities to link with the explosion mechanism of SN and multi-messenger observations.
Point
GASP 1Contact: Yusuke Tanimura (tanimura [at] nucl.phys.tohoku.ac.jp)