Speaker
Fumi Nakanishi
(Okayama University)
Description
We developed a new analysis method for supernova model identification using supernova neutrino observations in Super-Kamiokande (SK). Our new method uses some information on late-phase neutrinos observed in SK, such as the duration time of neutrino observation and averaged neutrino energy. In this presentation, we report the evaluation results of the supernova model identification performance.
| Submitted on behalf of a Collaboration? | No |
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Author
Fumi Nakanishi
(Okayama University)
Co-authors
Dr
Akira Harada
(RIKEN iTHEMS (Japan))
Prof.
Ken'ichiro Nakazato
(Faculty of Arts and Science, Kyushu University, Japan)
Prof.
Kohsuke Sumiyoshi
Dr
Masamitsu Mori
Mr
Masayuki Harada
Roger Wendell
Prof.
Yudai Suwa
Prof.
Yusuke Koshio
