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dc.contributor.authorAiello, Sebastiano
dc.contributor.authorAlbert, Arthur
dc.contributor.authorAlshamsi, Mohammed
dc.contributor.authorAlves Garre, Sergio
dc.contributor.authorAly, Zineb
dc.contributor.authorAmbrosone, Antonio
dc.contributor.authorAmeli, Fabrizio
dc.contributor.authorAndré, Michel
dc.contributor.authorAndroulakis, Giorgos
dc.contributor.authorAnghinolfi, Marco
dc.contributor.authorAnguita, M.
dc.contributor.authorArdid Ramírez, Miguel
dc.contributor.authorArdid Ramírez, Joan Salvador
dc.contributor.authorAublin, J.
dc.contributor.authorBagatelas, Christos
dc.contributor.otherUniversitat Politècnica de Catalunya. Departament de Física
dc.date.accessioned2024-02-27T13:42:06Z
dc.date.available2024-02-27T13:42:06Z
dc.date.issued2022-03-09
dc.identifier.citationAiello, S. [et al.]. Combined sensitivity of JUNO and KM3NeT/ORCA to the neutrino mass ordering. "Journal of high energy physics", 9 Març 2022, vol. 2022, núm. 3, article 55.
dc.identifier.issn1029-8479
dc.identifier.otherhttp://hdl.handle.net/10251/190456
dc.identifier.urihttp://hdl.handle.net/2117/403313
dc.description.abstractThis article presents the potential of a combined analysis of the JUNO and KM3NeT/ORCA experiments to determine the neutrino mass ordering. This combination is particularly interesting as it significantly boosts the potential of either detector, beyond simply adding their neutrino mass ordering sensitivities, by removing a degeneracy in the determination of ¿ between the two experiments when assuming the wrong ordering. The study is based on the latest projected performances for JUNO, and on simulation tools using a full Monte Carlo approach to the KM3NeT/ORCA response with a careful assessment of its energy systematics. From this analysis, a 5s determination of the neutrino mass ordering is expected after 6 years of joint data taking for any value of the oscillation parameters. This sensitivity would be achieved after only 2 years of joint data taking assuming the current global best-fit values for those parameters for normal ordering.
dc.description.sponsorshipThe authors acknowledge the financial support of the funding agencies: Agence Nationale de la Recherche (contract ANR-15-CE31-0020), Centre National de la Recherche Scientifique (CNRS), Commission Europeenne (FEDER fund and Marie Curie Program), Institut Universitaire de France (IUF), LabEx UnivEarthS (ANR-10-LABX-0023 and ANR-18-IDEX-0001), Shota Rustaveli National Science Foundation of Georgia (SRNSFG, FR18-1268), Georgia; Deutsche Forschungsgemeinschaft (DFG), Germany; The General Secretariat of Research and Technology (GSRT), Greece; Istituto Nazionale di Fisica Nucleare (INFN), Ministero dell'Universita e della Ricerca (MIUR), PRIN 2017 program (Grant NAT-NET 2017W4HA7S) Italy; Ministry of Higher Education Scientific Research and Professional Training, ICTP through Grant AF-13, Morocco; Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; The National Science Centre, Poland (2015/18/E/ST2/00758); National Authority for Scientific Research (ANCS), Romania; Ministerio de Ciencia, Innovacion, Investigacion y Universidades (MCIU): Programa Estatal de Generacion de Conocimiento (refs. PGC2018-096663-B-C41, -A-C42, -B-C43, -B-C44) (MCIU/FEDER), Generalitat Valenciana: Prometeo (PROMETEO/2020/019), Grisolia (ref. GRISOLIA/2018/119) and GenT (refs. CIDEGENT/2018/034,/2019/043,/2020/049) programs, Junta de Andalucia (ref. A-FQM-053-UGR18), La Caixa Foundation (ref. LCF/BQ/IN17/11620019), EU: MSC program (ref. 101025085), Spain.
dc.language.isoeng
dc.publisherSpringer
dc.rightsAttribution 4.0 International
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.subjectÀrees temàtiques de la UPC::Física::Astronomia i astrofísica
dc.subject.lcshNeutrinos
dc.subject.lcshOscillations
dc.subject.otherNeutrino Detectors and Telescopes (experiments)
dc.subject.otherOscillation
dc.titleCombined sensitivity of JUNO and KM3NeT/ORCA to the neutrino mass ordering
dc.typeArticle
dc.subject.lemacNeutrins
dc.subject.lemacOscil·lacions
dc.contributor.groupUniversitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques
dc.identifier.doi10.1007/JHEP03(2022)055
dc.description.peerreviewedPeer Reviewed
dc.relation.publisherversionhttps://link.springer.com/article/10.1007/JHEP03(2022)055
dc.rights.accessOpen Access
local.identifier.drac38178147
dc.description.versionPostprint (published version)
local.citation.authorAiello, S.; Albert, A.; Alshamsi, M.; Alves, S.; Zineb, A.; Ambrosone, A.; Ameli, F.; Andre, M.; Androulakis, G.; Anghinolfi, M.; Anguita, M.; Ardid, M.; Ardid, J.; Aublin, J.; Bagatelas, C.
local.citation.publicationNameJournal of high energy physics
local.citation.volume2022
local.citation.number3, article 55


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