Unfinished fabric of the three neutrino paradigm

dc.contributor.authorCapozzi, Francescoen
dc.contributor.authorDi Valentino, Eleonoraen
dc.contributor.authorLisi, Eligioen
dc.contributor.authorMarrone, Antonioen
dc.contributor.authorMelchiorri, Alessandroen
dc.contributor.authorPalazzo, Antonioen
dc.date.accessioned2021-12-02T15:46:12Zen
dc.date.available2021-12-02T15:46:12Zen
dc.date.issued2021-10-26en
dc.description.abstractIn the current 3. paradigm, neutrino flavor oscillations probe three mixing angles (theta(12),theta(23),theta(13)), one CP-violating phase d, and two independent differences between the squared masses m(i)(2), that can be chosen as delta m(2) = m(2)(2) - m(1)(2) > 0 and Delta m(2) = m(3)(2) - (m(1)(2) (m(2)(2))=2, where sign (Delta m(2)) = +(-) for normal (inverted) mass ordering. Absolute. masses can be probed by the effective mass m(beta) in beta decay, by the total mass S in cosmology and-if neutrinos are Majorana-by another effective mass m(beta beta) in neutrinoless double beta decay. Within an updated global analysis of oscillation and nonoscillation data, we constrain these 3. parameters, both separately and in selected pairs, and highlight the concordance or discordance among different constraints. Five oscillation parameters vertical bar delta m(2)broken vertical bar, vertical bar Delta m(2)vertical bar; theta(12); theta(23); theta(13)) are consistently measured, with an overall accuracy ranging from similar to 1% for j.m2 j to similar to 6% for sin2. 23 (due to its persisting octant ambiguity). We find overall hints for normal ordering (at similar to 2.5 sigma), as well as for theta(23) < pi/4 and for sin delta < 0 (both at 90% C.L.), and discuss some tensions among different datasets. Concerning nonoscillation data, we include the recent KATRIN constraints on m(beta), and we combine the latest Ge-76, Te-130 and Xe-136 bounds on m(beta beta), accounting for nuclear matrix element covariances. We also discuss some variants related to cosmic microwave background (CMB) anisotropy and lensing data, which may affect cosmological constraints on S and hints on sign(Delta m(2)). The default option, including all Planck results, irrespective of the so-called lensing anomaly, sets upper bounds on S at the level of similar to 10-1 eV, and further favors normal ordering up to similar to 3 sigma. An alternative option, that includes recent ACT results plus other independent results (from WMAP and selected Planck data) globally consistent with standard lensing, is insensitive to the ordering but prefers Sigma similar to few x 10(-1) eV, with different implications for m(beta) and m(beta beta) searches. In general, the unfinished fabric of the 3. paradigm appears to be at the junction of diverse searches in particle and nuclear physics, astrophysics and cosmology, whose convergence will be crucial to achieve a convincing completion.en
dc.description.notesWe are grateful to M. Nakahata for informing us about the latest public release of the Super-Kamiokande atmospheric neutrino (preliminary) analysis [20] . We thank L. Pandola and M. Sisti for useful discussions about 0 nu beta beta decay results. This work is partly supported by the Italian Ministero dell'Universita e Ricerca (MUR) through the research Grant No. 2017W4HA7S "NAT-NET: Neutrino and Astroparticle Theory Network" under the program PRIN 2017, and by the Istituto Nazionale di Fisica Nucleare (INFN) through the "Theoretical Astroparticle Physics" (TAsP) project. The work of F. C. is supported by the U.S. Department of Energy under the Award No. DE-SC0020250. E. D. V. acknowledges the support of the Addison-Wheeler Fellowship awarded by the Institute of Advanced Study at Durham University.en
dc.description.sponsorshipItalian Ministero dell'Universita e Ricerca (MUR)Ministry of Education, Universities and Research (MIUR) [2017W4HA7S]; Istituto Nazionale di Fisica Nucleare (INFN) through the "Theoretical Astroparticle Physics" (TAsP) project.; U.S. Department of EnergyUnited States Department of Energy (DOE) [DE-SC0020250]; Addison-Wheeler Fellowship - Institute of Advanced Study at Durham Universityen
dc.description.versionPublished versionen
dc.format.mimetypeapplication/pdfen
dc.identifier.doihttps://doi.org/10.1103/PhysRevD.104.083031en
dc.identifier.eissn2470-0029en
dc.identifier.issn2470-0010en
dc.identifier.issue8en
dc.identifier.other83031en
dc.identifier.urihttp://hdl.handle.net/10919/106814en
dc.identifier.volume104en
dc.language.isoenen
dc.rightsCreative Commons Attribution 4.0 Internationalen
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/en
dc.titleUnfinished fabric of the three neutrino paradigmen
dc.title.serialPhysical Review Den
dc.typeArticle - Refereeden
dc.type.dcmitypetexten

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