Nucleon Decays into Light New Particles in Neutrino Detectors

dc.contributor.authorHeeck, Julianen
dc.contributor.authorShoemaker, Ian M.en
dc.date.accessioned2025-09-22T13:36:52Zen
dc.date.available2025-09-22T13:36:52Zen
dc.date.issued2025-09-11en
dc.description.abstractProton and neutron decays into light new particles X can drastically change the experimental signatures and benefit from the complementarity of large water-Cherenkov neutrino detectors such as Super- and Hyper-Kamiokande and tracking detectors such as JUNO and DUNE. The proton decays p → 𝓁⁺X and p → π⁺X with mX near phase-space closure lead to charged particles below the Cherenkov threshold, rendering them practically invisible in Super- and Hyper-Kamiokande but not in JUNO and DUNE, which are therefore uniquely positioned for these baryon-number-violating signatures despite their smaller size. As an additional signature, such nucleon decays in the Earth can produce a sizable flux of X particles in underground detectors.We present a simple model in which nucleons decay into sub-GeV sterile neutrinos that subsequently decay through active-sterile neutrino mixing, with a promisingly large number of events in Super-Kamiokande even in the seesaw-motivated parameter space.en
dc.description.sponsorshipThis work was supported by a 4-VA at UVA Collaborative Research Grant and by the U.S. Department of Energy under Grants No. DE-SC0007974 (J. H.) and No. DE-SC0020262 (I. M. S.).en
dc.description.versionPublished versionen
dc.format.mimetypeapplication/pdfen
dc.identifier.doihttps://doi.org/10.1103/cxvm-p412en
dc.identifier.urihttps://hdl.handle.net/10919/137812en
dc.identifier.volume135en
dc.language.isoenen
dc.publisherAmerican Physical Societyen
dc.rightsCreative Commons Attribution 4.0 Internationalen
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/en
dc.titleNucleon Decays into Light New Particles in Neutrino Detectorsen
dc.title.serialPhysical Review Lettersen
dc.typeArticle - Refereeden
dc.type.dcmitypeTexten

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