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2020 global reassessment of the neutrino oscillation picture

dc.contributor.authorde Salas P.F
dc.contributor.authorForero D.V
dc.contributor.authorGariazzo S
dc.contributor.authorMartínez-Miravé P
dc.contributor.authorMena O
dc.contributor.authorTernes C.A
dc.contributor.authorTórtola M
dc.contributor.authorValle J.W.F.
dc.date.accessioned2022-09-14T14:33:25Z
dc.date.available2022-09-14T14:33:25Z
dc.date.created2021
dc.identifier.issn10298479
dc.identifier.urihttp://hdl.handle.net/11407/7359
dc.descriptionWe present an updated global fit of neutrino oscillation data in the simplest three-neutrino framework. In the present study we include up-to-date analyses from a number of experiments. Concerning the atmospheric and solar sectors, besides the data considered previously, we give updated analyses of IceCube DeepCore and Sudbury Neutrino Observatory data, respectively. We have also included the latest electron antineutrino data collected by the Daya Bay and RENO reactor experiments, and the long-baseline T2K and NOνA measurements, as reported in the Neutrino 2020 conference. All in all, these new analyses result in more accurate measurements of θ13, θ12, Δm212 and |Δm312|. The best fit value for the atmospheric angle θ23 lies in the second octant, but first octant solutions remain allowed at ∼ 2.4σ. Regarding CP violation measurements, the preferred value of δ we obtain is 1.08π (1.58π) for normal (inverted) neutrino mass ordering. The global analysis still prefers normal neutrino mass ordering with 2.5σ statistical significance. This preference is milder than the one found in previous global analyses. These new results should be regarded as robust due to the agreement found between our Bayesian and frequentist approaches. Taking into account only oscillation data, there is a weak/moderate preference for the normal neutrino mass ordering of 2.00σ. While adding neutrinoless double beta decay from the latest Gerda, CUORE and KamLAND-Zen results barely modifies this picture, cosmological measurements raise the preference to 2.68σ within a conservative approach. A more aggressive data set combination of cosmological observations leads to a similar preference for normal with respect to inverted mass ordering, namely 2.70σ. This very same cosmological data set provides 2σ upper limits on the total neutrino mass corresponding to Σmν< 0.12 (0.15) eV in the normal (inverted) neutrino mass ordering scenario. The bounds on the neutrino mixing parameters and masses presented in this up-to-date global fit analysis include all currently available neutrino physics inputs. © 2021, The Author(s).eng
dc.language.isoeng
dc.publisherSpringer Science and Business Media Deutschland GmbH
dc.relation.isversionofhttps://www.scopus.com/inward/record.uri?eid=2-s2.0-85107338184&doi=10.1007%2fJHEP02%282021%29071&partnerID=40&md5=bf4fb8d26f5ecc39bb07cfee41a12aa7
dc.sourceJournal of High Energy Physics
dc.title2020 global reassessment of the neutrino oscillation picture
dc.typeArticle
dc.rights.accessrightsinfo:eu-repo/semantics/restrictedAccess
dc.publisher.programCiencias Básicas
dc.type.spaArtículo
dc.identifier.doi10.1007/JHEP02(2021)071
dc.subject.keywordBeyond Standard Modeleng
dc.subject.keywordNeutrino Physicseng
dc.relation.citationvolume2021
dc.relation.citationissue2
dc.publisher.facultyFacultad de Ciencias Básicas
dc.affiliationde Salas, P.F., The Oskar Klein Centre for Cosmoparticle Physics, Department of Physics, Stockholm University, AlbaNova, Stockholm, 10691, Sweden
dc.affiliationForero, D.V., Universidad de Medellín, Carrera 87 No, Medellín, 30-65, Colombia
dc.affiliationGariazzo, S., Instituto de Física Corpuscular, CSIC-Universitat de València, Paterna, 46980, Spain, INFN, Sezione di Torino, Via P. Giuria 1, Torino, I-10125, Italy
dc.affiliationMartínez-Miravé, P., Instituto de Física Corpuscular, CSIC-Universitat de València, Paterna, 46980, Spain, Departament de Física Teòrica, Universitat de València, Burjassot, 46100, Spain
dc.affiliationMena, O., Instituto de Física Corpuscular, CSIC-Universitat de València, Paterna, 46980, Spain
dc.affiliationTernes, C.A., Instituto de Física Corpuscular, CSIC-Universitat de València, Paterna, 46980, Spain, INFN, Sezione di Torino, Via P. Giuria 1, Torino, I-10125, Italy
dc.affiliationTórtola, M., Instituto de Física Corpuscular, CSIC-Universitat de València, Paterna, 46980, Spain, Departament de Física Teòrica, Universitat de València, Burjassot, 46100, Spain
dc.affiliationValle, J.W.F., Instituto de Física Corpuscular, CSIC-Universitat de València, Paterna, 46980, Spain
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dc.type.coarhttp://purl.org/coar/resource_type/c_6501
dc.type.versioninfo:eu-repo/semantics/publishedVersion
dc.type.driverinfo:eu-repo/semantics/article
dc.identifier.reponamereponame:Repositorio Institucional Universidad de Medellín
dc.identifier.repourlrepourl:https://repository.udem.edu.co/
dc.identifier.instnameinstname:Universidad de Medellín


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