New Spallation Background Rejection Techniques to Greatly Improve the Solar Neutrino Sensitivity of JUNO
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| Format: | Preprint |
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2025
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| _version_ | 1866918160787046400 |
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| author | Nairat, Obada Beacom, John F. Li, Shirley Weishi |
| author_facet | Nairat, Obada Beacom, John F. Li, Shirley Weishi |
| contents | While the potential of the Jiangmen Underground Neutrino Observatory (JUNO) to measure solar neutrinos is known, realizing this potential requires new techniques to reduce detector backgrounds. One of the most serious backgrounds is due to the beta decays of unstable nuclei produced through muon breakup (spallation) of nuclei. This background is much more significant in JUNO compared to Super-Kamiokande due to JUNO's shallower depth and its lack of directional information. We present the first detailed theoretical calculations of spallation backgrounds in JUNO, showing the underlying physical processes and new ways to cut backgrounds while preserving signals. A key point is showing the importance of neutron tagging to identify hadronic showers, which are rare but produce almost all of the dangerous isotopes. With our new techniques, JUNO will be able to reduce deadtime (signal loss) by a factor of five and to reduce the running time needed to meet sensitivity goals by a factor of two. This will give JUNO greatly improved sensitivity to $^8$B and $hep$ solar neutrinos, as we will explore in a separate paper. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2510_12873 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | New Spallation Background Rejection Techniques to Greatly Improve the Solar Neutrino Sensitivity of JUNO Nairat, Obada Beacom, John F. Li, Shirley Weishi High Energy Physics - Phenomenology High Energy Astrophysical Phenomena High Energy Physics - Experiment Nuclear Experiment Nuclear Theory Instrumentation and Detectors While the potential of the Jiangmen Underground Neutrino Observatory (JUNO) to measure solar neutrinos is known, realizing this potential requires new techniques to reduce detector backgrounds. One of the most serious backgrounds is due to the beta decays of unstable nuclei produced through muon breakup (spallation) of nuclei. This background is much more significant in JUNO compared to Super-Kamiokande due to JUNO's shallower depth and its lack of directional information. We present the first detailed theoretical calculations of spallation backgrounds in JUNO, showing the underlying physical processes and new ways to cut backgrounds while preserving signals. A key point is showing the importance of neutron tagging to identify hadronic showers, which are rare but produce almost all of the dangerous isotopes. With our new techniques, JUNO will be able to reduce deadtime (signal loss) by a factor of five and to reduce the running time needed to meet sensitivity goals by a factor of two. This will give JUNO greatly improved sensitivity to $^8$B and $hep$ solar neutrinos, as we will explore in a separate paper. |
| title | New Spallation Background Rejection Techniques to Greatly Improve the Solar Neutrino Sensitivity of JUNO |
| topic | High Energy Physics - Phenomenology High Energy Astrophysical Phenomena High Energy Physics - Experiment Nuclear Experiment Nuclear Theory Instrumentation and Detectors |
| url | https://arxiv.org/abs/2510.12873 |