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dc.contributor.authorGarcía Gámez, Diego 
dc.contributor.authorNicolás Arnaldos, Francisco Javier 
dc.contributor.authorZamorano García, Bruno 
dc.contributor.authorThe Dune Collaboration
dc.identifier.citationThe DUNE collaboration et al. Searching for solar KDAR with DUNE. JCAP10 (2021) 065. [doi: 10.1088/1475-7516/2021/10/065]es_ES
dc.descriptionThis document was prepared by the DUNE collaboration using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. This work was supported by CNPq, FAPERJ, FAPEG and FAPESP, Brazil; CFI, IPP and NSERC, Canada; CERN; MŠMT, Czech Repub lic; ERDF, H2020-EU and MSCA, European Union; CNRS/IN2P3 and CEA, France; INFN, Italy; FCT, Portugal; NRF, South Korea; CAM, Fundación “La Caixa”, Junta de Andalucía FEDER, and MICINN, Spain; SERI and SNSF, Switzerland; TÜBİTAK, Turkey; The Royal Society and UKRI/STFC, United Kingdom; DOE and NSF, United States of America. We are grateful to Xerxes Tata for useful discussions. C. Rott acknowledges support from the National Research Foundation of Korea.es_ES
dc.description.abstractThe observation of 236 MeV muon neutrinos from kaon-decay-at-rest (KDAR) originating in the core of the Sun would provide a unique signature of dark matter annihilation. Since excellent angle and energy reconstruction are necessary to detect this monoenergetic, directional neutrino flux, DUNE with its vast volume and reconstruction capabilities, is a promising candidate for a KDAR neutrino search. In this work, we evaluate the proposed KDAR neutrino search strategies by realistically modeling both neutrino-nucleus interactions and the response of DUNE. We find that, although reconstruction of the neutrino energy and direction is difficult with current techniques in the relevant energy range, the superb energy resolution, angular resolution, and particle identification offered by DUNE can still permit great signal/background discrimination. Moreover, there are non-standard scenarios in which searches at DUNE for KDAR in the Sun can probe dark matter interactions.es_ES
dc.description.sponsorshipFermi National Accelerator Laboratory (Fermilab) No. DE-AC02-07CH11359.es_ES
dc.description.sponsorshipCNPq, FAPERJ, FAPEG y FAPESP, Brasiles_ES
dc.description.sponsorshipCFI, IPP y NSERC, Canadáes_ES
dc.description.sponsorshipMŠMT, República Checaes_ES
dc.description.sponsorshipMSCA, Unión Europeaes_ES
dc.description.sponsorshipCNRS/IN2P3 y CEA, Franciaes_ES
dc.description.sponsorshipINFN, Italiaes_ES
dc.description.sponsorshipFCT, Portugales_ES
dc.description.sponsorshipNRF, Corea del Sures_ES
dc.description.sponsorshipCAM, Fundación "La Caixa"es_ES
dc.description.sponsorshipJunta de Andalucía FEDER, y MICINN, Españaes_ES
dc.description.sponsorshipSERI y SNSF, Suizaes_ES
dc.description.sponsorshipTübİTAK, Turquíaes_ES
dc.description.sponsorshipLa Real Sociedad y UKRI/STFC, Reino Unidoes_ES
dc.description.sponsorshipDOE y NSF, Estados Unidos de Américaes_ES
dc.rightsAtribución 3.0 España*
dc.subjectDark matter theoryes_ES
dc.subjectNeutrino detectorses_ES
dc.titleSearching for solar KDAR with DUNEes_ES

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Atribución 3.0 España
Except where otherwise noted, this item's license is described as Atribución 3.0 España