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dc.contributor.authorAbud, A. Abed
dc.contributor.authorDUNE Collaboration
dc.contributor.authorFernández Martínez, L. Enrique 
dc.contributor.authorGonzález López, Manuel 
dc.contributor.authorRosauro Alcaraz, Salvador 
dc.contributor.otherUAM. Departamento de Física Teóricaes_ES
dc.date.accessioned2023-02-06T13:29:16Z
dc.date.available2023-02-06T13:29:16Z
dc.date.issued2022-04-25
dc.identifier.citationPhysical Review D 105.7 (2022): 072006es_ES
dc.identifier.issn2470-0010 (print)es_ES
dc.identifier.issn2470-0029 (online)es_ES
dc.identifier.urihttp://hdl.handle.net/10486/706199
dc.descriptionArtículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAMes_ES
dc.description.abstractThe Deep Underground Neutrino Experiment (DUNE) will produce world-leading neutrino oscillation measurements over the lifetime of the experiment. In this work, we explore DUNE's sensitivity to observe charge-parity violation (CPV) in the neutrino sector, and to resolve the mass ordering, for exposures of up to 100 kiloton-megawatt-calendar years (kt-MW-CY), where calendar years include an assumption of 57% accelerator uptime based on past accelerator performance at Fermilab. The analysis includes detailed uncertainties on the flux prediction, the neutrino interaction model, and detector effects. We demonstrate that DUNE will be able to unambiguously resolve the neutrino mass ordering at a 4σ (5σ) level with a 66 (100) kt-MW-CY far detector exposure, and has the ability to make strong statements at significantly shorter exposures depending on the true value of other oscillation parameters, with a median sensitivity of 3σ for almost all true δCP values after only 24 kt-MW-CY. We also show that DUNE has the potential to make a robust measurement of CPV at a 3σ level with a 100 kt-MW-CY exposure for the maximally CP-violating values δCP = ±π/2. Additionally, the dependence of DUNE's sensitivity on the exposure taken in neutrino-enhanced and antineutrino-enhanced running is discussed. An equal fraction of exposure taken in each beam mode is found to be close to optimal when considered over the entire space of interestes_ES
dc.format.extent32 pag.es_ES
dc.format.mimetypeapplication/pdfes_ES
dc.language.isoenges_ES
dc.publisherAmerican Physical Societyes_ES
dc.relation.ispartofPhysical Review D - Particles, Fields, Gravitation, and Cosmologyes_ES
dc.rights© 2022 authorses_ES
dc.subject.otherDetectores_ES
dc.subject.otherMesonses_ES
dc.subject.otherFermilabes_ES
dc.titleLow exposure long-baseline neutrino oscillation sensitivity of the DUNE experimentes_ES
dc.typearticlees_ES
dc.subject.ecienciaFísicaes_ES
dc.relation.publisherversionhttps://doi.org/10.1103/PhysRevD.105.072006es_ES
dc.identifier.doi10.1103/PhysRevD.105.072006es_ES
dc.identifier.publicationfirstpage072006-1es_ES
dc.identifier.publicationissue7es_ES
dc.identifier.publicationlastpage072006-32es_ES
dc.identifier.publicationvolume105es_ES
dc.type.versioninfo:eu-repo/semantics/publishedVersiones_ES
dc.rights.ccReconocimientoes_ES
dc.rights.accessRightsopenAccesses_ES
dc.facultadUAMFacultad de Cienciases_ES
dc.institutoUAMInstituto de Física Teórica (IFT)es_ES


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