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dc.contributor.authorChauhan, Bhavesh-
dc.date.accessioned2024-08-20T06:52:39Z-
dc.date.available2024-08-20T06:52:39Z-
dc.date.issued2022-05-
dc.identifier.urihttps://journals.aps.org/prd/abstract/10.1103/PhysRevD.105.095035-
dc.identifier.urihttp://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/15290-
dc.description.abstractLarge liquid scintillator detectors, such as JUNO, present a new opportunity to study neutral current events from the low-energy end of the atmospheric neutrinos, and possible new physics signals due to light dark matter. We carefully study the possibility of detecting “large-energy singles” (LES), i.e., events with visible scintillation energy >15  MeV, but no other associated tags. For an effective exposure of 20  kton−yr and considering only Standard Model physics, we expect the LES sample to contain ∼40 events from scattering on free protons and ∼108 events from interaction with carbon, from neutral-current interactions of atmospheric neutrinos. Backgrounds, largely due to 𝛽 decays of cosmogenic isotopes, are shown to be significant only below 15 MeV visible energy. The LES sample at JUNO can competitively probe a variety of new physics scenarios, such as boosted dark matter and annihilation of galactic dark matter to sterile neutrinos.en_US
dc.language.isoenen_US
dc.publisherAPSen_US
dc.subjectPhysicsen_US
dc.subjectJUNOen_US
dc.subjectSolar and atmospheric neutrinosen_US
dc.titleLarge-energy single hits at JUNO from atmospheric neutrinos and dark matteren_US
dc.typeArticleen_US
Appears in Collections:Department of Physics

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