Pulsational Pair-instability Supernovae. II. Neutrino Signals from Pulsations and their Detection by Terrestrial Neutrino Detectors

A Pulsational Pair-instability supernova (PPISN) evolves from a massive star with a mass \(\sim 80\) -- 140 \(M_{\odot}\) which develops the electron-positron pair-instability after the hydrostatic He-burning in the core has finished. In [Leung et al., ApJ 887, 72 (2019)] (Paper I) we examined the e...

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Veröffentlicht in:	arXiv.org 2020-07
Hauptverfasser:	Shing-Chi Leung, Blinnikov, Sergei, Ishidoshiro, Koji, Kozlov, Alexandre, Nomoto, Ken'ichi
Format:	Artikel
Sprache:	eng
Schlagworte:	Detectors Emission analysis Light curve Massive stars Neutrinos Optical communication Physics - High Energy Astrophysical Phenomena Stability Supernovae Telescopes
Online-Zugang:	Volltext
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