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Published in 2019 at "Physical Review D"
DOI: 10.1103/physrevd.100.063018
Abstract: Rotation of core-collapse supernovae (SNe) affects the neutrino emission characteristics. By comparing the neutrino properties of three three-dimensional SN simulations of a 15 M_sun progenitor (one non-rotating model and two models rotating at different velocities),…
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Keywords:
standing accretion;
accretion shock;
neutrino;
shock instability ... See more keywords