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dc.contributor.authorChauhan, Bhavesh-
dc.date.accessioned2024-08-20T04:32:33Z-
dc.date.available2024-08-20T04:32:33Z-
dc.date.issued2021-11-
dc.identifier.urihttps://link.aps.org/pdf/10.1103/PhysRevD.105.095035-
dc.identifier.urihttp://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/15284-
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.publisherAmerican Physical Societyen_US
dc.subjectPhysicsen_US
dc.subjectHigh Energy Physics - Phenomenology (hep-ph)en_US
dc.subjectJUNOen_US
dc.subjectLarge Energy Singlesen_US
dc.titleLarge Energy Singles at JUNO from Atmospheric Neutrinos and Dark Matteren_US
dc.typeArticleen_US
Appears in Collections:Department of Physics

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