Volume 441 -
XVIII International Conference on Topics in Astroparticle and Underground Physics (TAUP2023) -
Neutrino Physics and Astrophysics
Development of analysis method for late-phase neutrino emission from the supernova in Super-Kamiokande
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Pre-published on:
February 16, 2024
Published on:
March 22, 2024
Abstract
A new analysis method for supernova model identification using supernova neutrino observations in Super-Kamiokande (SK) is developed. This new method uses information on late-phase neutrinos observed in SK, such as the duration of supernova neutrino and average neutrino energy. In this paper, we report the evaluation results of the supernova identification performance, demonstrating 90% or more in identification performance.
DOI: https://doi.org/10.22323/1.441.0209
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.