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dc.contributor.authorHernández, Eliecer-
dc.contributor.authorNieves, Juan Miguel-
dc.contributor.authorSanchez, F.-
dc.contributor.authorSobczyk, J.E.-
dc.date.accessioned2023-10-04T11:50:02Z-
dc.date.available2023-10-04T11:50:02Z-
dc.date.issued2022-06-
dc.identifierdoi: 10.1016/j.physletb.2022.137046-
dc.identifierissn: 0370-2693-
dc.identifier.citationPHYSICS LETTERS B 829: 137046 (2022)-
dc.identifier.urihttp://hdl.handle.net/10261/336529-
dc.description.abstractSince the ν(ν¯)A→τX reaction is notoriously difficult to be directly measured, the information on the dynamics of this nuclear process should be extracted from the analysis of the energy and angular distributions of the tau decay visible products. These distributions depend, in addition to dσ/(dEdcos⁡θ), on the components of the tau-polarization vector. We give, for the first time, the general expression for the outgoing hadron (pion or rho meson) energy and angular differential cross section for the sequential νA→τ(πν,ρν)X and ν¯A→τ(πν¯,ρν¯)X reactions. Though all possible nuclear reaction mechanisms contribute to the distribution, it may be possible to isolate/enhance one of them by implementing appropriate selection criteria. For the case of the quasi-elastic reaction off oxygen and neutrino energies below 6 GeV, we show that the pion distributions are quite sensitive to the details of the tau-polarization components. We find significant differences between the full calculation, where the longitudinal and transverse components of the tau polarization vector vary with the energy and the scattering angle of the produced tau, and the simplified scheme in which the polarizations are set to one and zero, being the latter their respective asymptotic values reached in the high energy regime. In addition to its potential impact on neutrino oscillation analyses, this result can be used to further test different nuclear models, since these observables provide complementary information to that obtained by means of the inclusive nuclear weak charged-current differential cross section. We also study the effects on the cross section of the W and W nuclear structure functions, which contributions are proportional to the charged lepton mass, and therefore difficult to constrain in muon and electron neutrino experiments.-
dc.description.sponsorshipThis research has been supported by the Spanish Ministerio de Ciencia e Innovación (MICINN) and the European Regional Development Fund (ERDF) under contracts FIS2017-84038-C2-1-P, PID2020-112777GB-I00 and PID2019-105439G-C22, the EU STRONG-2020 project under the program H2020-INFRAIA-2018-1, grant agreement no. 824093 and by Generalitat Valenciana under contract PROMETEO/2020/023, the Deutsche Forschungsgemeinschaft (DFG) through the Cluster of Excellence “Precision Physics, Fundamental Interactions, and Structure of Matter” (PRISMA+EXC 2118/1) funded by the DFG within the German Excellence Strategy (Project ID 39083149) and the Swiss National Foundation under the grant 200021_85012.-
dc.languageeng-
dc.publisherElsevier BV-
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/FIS2017-84038-C2-1-P/ES/TEORIAS EFECTIVAS EN FISICA NUCLEAR Y DE HADRONES/-
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2020-112777GB-I00/ES/FISICA NUCLEAR Y HADRONICA A ENERGIAS INTERMEDIAS/-
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-105439GB-C22/ES/FISICA HADRONICA, INTERACCIONES FUNDAMENTALES Y FISICA NUCLEAR/-
dc.relationinfo:eu-repo/grantAgreement/EC/H2020/824093 (H2020-INFRAIA-2018-1)-
dc.relationinfo:eu-repo/grantAgreement/GVA//PROMETEO/2020/023,-
dc.relation.isversionofPublisher's version-
dc.rightsopenAccess-
dc.titleTau longitudinal and transverse polarizations from visible kinematics in (anti-)neutrino nucleus scattering-
dc.typeartículo-
dc.identifier.doi10.1016/j.physletb.2022.137046es_ES
dc.relation.publisherversionhttp://dx.doi.org/10.1016/j.physletb.2022.137046-
dc.date.updated2023-10-04T11:50:02Z-
dc.rights.licensehttps://creativecommons.org/licenses/by/4.0/-
dc.contributor.funderEuropean Commission-
dc.contributor.funderMinisterio de Ciencia e Innovación (España)-
dc.contributor.funderGeneralitat Valenciana-
dc.contributor.funderAgencia Estatal de Investigación (España)-
dc.relation.csic-
dc.identifier.funderhttp://dx.doi.org/10.13039/501100004837es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100003359es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100000780es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100011033es_ES
local.message.claim2023-12-20T14:40:06.394+0100|||rp15217|||submit_approve|||dc_contributor_author|||None*
dc.type.coarhttp://purl.org/coar/resource_type/c_6501es_ES
item.grantfulltextopen-
item.fulltextWith Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
item.openairetypeartículo-
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