Parametrizing the reconstruction performance of Super-Kamiokande in the Sub-GeV to TeV neutrino energy range
Fuente:
arXiv
Salvato in:
| Autore principale: | |
|---|---|
| Natura: | Preprint |
| Pubblicazione: |
2025
|
| Soggetti: | |
| Accesso online: | |
| Tags: |
Aggiungi Tag
Nessun Tag, puoi essere il primo ad aggiungerne!!
|
| _version_ | 1866909624830001152 |
|---|---|
| author | Jesús-Valls, C. |
| author_facet | Jesús-Valls, C. |
| contents | Super-Kamiokande is a paramount detector for studying atmospheric, astrophysical and accelerator neutrino physics. This work extracts and characterizes the neutrino reconstruction performance of Super-Kamiokande using the public data release from its latest atmospheric neutrino analysis. Energy and zenith angle reconstruction performances are derived and modeled for neutrinos spanning sub-GeV to TeV energies across different event samples and sample-specific and sample-aggregated performances are provided. These metrics enable realistic detector response modeling in phenomenological studies, establish benchmarks for evaluating alternative reconstruction algorithms, facilitate quantitative performance comparisons with other experiments, and provide a baseline performance model for the future Hyper-Kamiokande detector. This study represents the first publicly available comprehensive model to describe neutrino reconstruction in Super-Kamiokande in the Sub-GeV to TeV energies. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2505_20812 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Parametrizing the reconstruction performance of Super-Kamiokande in the Sub-GeV to TeV neutrino energy range Jesús-Valls, C. High Energy Physics - Experiment Instrumentation and Detectors Super-Kamiokande is a paramount detector for studying atmospheric, astrophysical and accelerator neutrino physics. This work extracts and characterizes the neutrino reconstruction performance of Super-Kamiokande using the public data release from its latest atmospheric neutrino analysis. Energy and zenith angle reconstruction performances are derived and modeled for neutrinos spanning sub-GeV to TeV energies across different event samples and sample-specific and sample-aggregated performances are provided. These metrics enable realistic detector response modeling in phenomenological studies, establish benchmarks for evaluating alternative reconstruction algorithms, facilitate quantitative performance comparisons with other experiments, and provide a baseline performance model for the future Hyper-Kamiokande detector. This study represents the first publicly available comprehensive model to describe neutrino reconstruction in Super-Kamiokande in the Sub-GeV to TeV energies. |
| title | Parametrizing the reconstruction performance of Super-Kamiokande in the Sub-GeV to TeV neutrino energy range |
| topic | High Energy Physics - Experiment Instrumentation and Detectors |
| url | https://arxiv.org/abs/2505.20812 |