Saved in:
| Main Authors: | , , , |
|---|---|
| Format: | Preprint |
| Published: |
2024
|
| Subjects: | |
| Online Access: | https://arxiv.org/abs/2402.00283 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1866916111937699840 |
|---|---|
| author | Nakanishi, Fumi Izumiyama, Shota Harada, Masayuki Koshio, Yusuke |
| author_facet | Nakanishi, Fumi Izumiyama, Shota Harada, Masayuki Koshio, Yusuke |
| contents | If a galactic supernova explosion occurs in the future, it will be critical to rapidly alert the community to the direction of the supernova by utilizing neutrino signals in order to enable the initiation of follow-up optical observations. In addition, there is anticipation that observation of the diffuse supernova neutrino background will yield discoveries in the near future, given that experimental upper limits are approaching theoretical predictions. We have developed a new supernova event simulator for water Cherenkov neutrino detectors, such as the highly sensitive Super-Kamiokande. This simulator calculates the neutrino interaction in water for the two types of supernova neutrinos described above. Its purpose is to evaluate the precision in determining the location of supernovae and to estimate the expected number of events related to the diffuse supernova neutrino background in Super-Kamiokande. In this paper, we describe the basic structure of the simulator and its demonstration. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2402_00283 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Supernova burst and Diffuse Supernova Neutrino Background simulator for Water Cherenkov Detectors Nakanishi, Fumi Izumiyama, Shota Harada, Masayuki Koshio, Yusuke Instrumentation and Methods for Astrophysics If a galactic supernova explosion occurs in the future, it will be critical to rapidly alert the community to the direction of the supernova by utilizing neutrino signals in order to enable the initiation of follow-up optical observations. In addition, there is anticipation that observation of the diffuse supernova neutrino background will yield discoveries in the near future, given that experimental upper limits are approaching theoretical predictions. We have developed a new supernova event simulator for water Cherenkov neutrino detectors, such as the highly sensitive Super-Kamiokande. This simulator calculates the neutrino interaction in water for the two types of supernova neutrinos described above. Its purpose is to evaluate the precision in determining the location of supernovae and to estimate the expected number of events related to the diffuse supernova neutrino background in Super-Kamiokande. In this paper, we describe the basic structure of the simulator and its demonstration. |
| title | Supernova burst and Diffuse Supernova Neutrino Background simulator for Water Cherenkov Detectors |
| topic | Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2402.00283 |