Three-dimensional supernova simulation of SN 1987A progenitor with implications for multi-messenger signals

¹ Department of Applied Physics, Fukuoka University, Fukuoka 814-0180, Japan
² Research Institute of Stellar Explosive Phenomena, Fukuoka University, Fukuoka 814-0180, Japan

^* e-mail: nakamurako@fukuoka-u.ac.jp

Published online: 24 February 2022

Abstract

Recently a new progenitor model for SN 1987A has been constructed. This progenitor model is based on a slow-merger of 14 M_⊙ and 9 M_⊙ stars and it satisfies most of the observational constraints such as red-toblue evolution, lifetime, total mass and position in the Hertzsprung-Russell diagram at collapse, and chemical anomalies. We perform a three-dimensional self-consistent core-collapse supernova simulation using this new progenitor model and find that it successfully presents an explosion and leaves a 1.53 M_⊙ neutron star. Assuming a detector sensitivity of Kamiokande-II and the distance to the supernova of 51 kpc, we obtain 16 neutrino detection events in one second. Some characteristic modes in its gravitational wave signal are also discussed in this article.