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Neutron Tagging Can Greatly Reduce Spallation Backgrounds in Super-Kamiokande

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arxiv 2409.10611 v2 pith:KFVMSCYW submitted 2024-09-16 hep-ph astro-ph.HEhep-exnucl-exnucl-th

classification hep-phastro-ph.HEhep-exnucl-exnucl-th
keywords backgroundssuper-kamiokandeshowersspallationcutsdepthdetectorfurther
verification ladder T0 review T1 audit T2 compute T3 formal
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Super-Kamiokande's spallation backgrounds - the delayed beta decays of nuclides following cosmic-ray muons - are nearly all produced by the small fraction of muons with hadronic showers. We show that these hadronic showers also produce neutrons; their captures can be detected with high efficiency due to the recent addition of dissolved gadolinium to Super-Kamiokande. We show that new cuts based on the neutron tagging of showers could reduce spallation backgrounds by a factor of at least four beyond present cuts. With further work, this could lead to a near-elimination of detector backgrounds above about 6 MeV, which would significantly improve the sensitivity of Super-Kamiokande. These findings heighten the importance of adding gadolinium to Hyper-Kamiokande, which is at a shallower depth. Further, a similar approach could be used in other detectors, for example, the JUNO liquid-scintillator detector, which is also at a shallower depth.

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  1. Search for Diffuse Supernova Neutrino Background with 956.2 days of Super-Kamiokande Gadolinium Dataset

    astro-ph.HE 2025-11 accept novelty 6.0 of 10

    No significant diffuse supernova neutrino background signal was found in 956.2 days of SK-Gd data; new 90% upper limits were set on the astrophysical electron antineutrino flux.

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