PoS - Proceedings of Science
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
F. Nakanishi*, A. Harada, M. Harada, Y. Koshio, M. Mori, K.i. Nakazato, K. Sumiyoshi, Y. Suwa and R. A. Wendell
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Pre-published on: February 16, 2024
Published on: March 22, 2024
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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