dc.creator | González Jiménez, Raúl | es |
dc.creator | Barbaro, M. B | es |
dc.creator | Caballero Carretero, Juan Antonio | es |
dc.creator | Donnelly, T. W. | es |
dc.creator | Jachowicz, N. | es |
dc.creator | Megías Vázquez, Guillermo Daniel | es |
dc.creator | Niewczas, K. | es |
dc.creator | Nikolakopoulos, A. | es |
dc.creator | Van Orden, J. W. | es |
dc.creator | Udías, J. M. | es |
dc.date.accessioned | 2023-01-16T19:28:26Z | |
dc.date.available | 2023-01-16T19:28:26Z | |
dc.date.issued | 2022 | |
dc.identifier.citation | González Jiménez, R., Barbaro, M.B., Caballero Carretero, J.A., Donnelly, T.W., Jachowicz, N., Megías Vázquez, G.D.,...,Udías, J.M. (2022). Neutrino Energy Reconstruction from Semi-inclusive Samples. Physical Review C, 105 (2), 025502. https://doi.org/10.1103/PhysRevC.105.025502. | |
dc.identifier.issn | 2469-9985 | es |
dc.identifier.issn | 2469-9993 | es |
dc.identifier.uri | https://hdl.handle.net/11441/141412 | |
dc.description.abstract | We study neutrino-nucleus charged-current reactions on finite nuclei for the situation in which an outgoing muon and a proton are detected in coincidence; i.e., we focus on semi-inclusive cross sections. We limit our attention to one-body current interactions (quasielastic scattering) and assess the impact of different nuclear effects in the determination of the neutrino energy. We identify the regions in phase space where the neutrino energy can be reconstructed relatively well and study whether the cross section in those regions is significant. Our results indicate that it is possible to filter more than 50% of all events according to the muon and proton kinematics, so that for the DUNE and T2K fluxes the neutrino energy can be determined with uncertainties of less than 1% and 3%, respectively. Furthermore, we find that the reconstructed neutrino energy does not depend strongly on how one treats the final-state interactions and is not much affected by the description of the initial state. On the other hand, the estimations of the uncertainty on the neutrino energy show important sensitivity to the modeling of the initial state. | es |
dc.description.sponsorship | United States Department of Energy DE-AC05-06OR23177 | es |
dc.description.sponsorship | Universidad Complutense de Madrid PR65/19-22430 | es |
dc.description.sponsorship | University of Turin BARM-RILO-18-02 | es |
dc.description.sponsorship | Ministerio de Economía y Competitividad FIS2017-88410-P | es |
dc.description.sponsorship | European Commission FIS2017-88410-P | es |
dc.description.sponsorship | Junta de Andalucia FQM160, SOMM17/6105/UGR | es |
dc.description.sponsorship | University of Tokyo A07 | es |
dc.description.sponsorship | NCN Preludium 2020/37/N/ST2/01751 | es |
dc.description.sponsorship | Ministry of Science and Higher Education, Poland DIR WK/2017/05 | es |
dc.description.sponsorship | SKA South Africa 839481 | es |
dc.format | application/pdf | es |
dc.format.extent | 16 p. | es |
dc.language.iso | eng | es |
dc.publisher | American Physical Society | es |
dc.relation.ispartof | Physical Review C, 105 (2), 025502. | |
dc.rights | Attribution-NonCommercial-NoDerivatives 4.0 Internacional | * |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/4.0/ | * |
dc.title | Neutrino Energy Reconstruction from Semi-inclusive Samples | es |
dc.type | info:eu-repo/semantics/article | es |
dcterms.identifier | https://ror.org/03yxnpp24 | |
dc.type.version | info:eu-repo/semantics/publishedVersion | es |
dc.rights.accessRights | info:eu-repo/semantics/openAccess | es |
dc.contributor.affiliation | Universidad de Sevilla. Departamento de Física Atómica, Molecular y Nuclear | es |
dc.relation.projectID | DE-AC05-06OR23177 | es |
dc.relation.projectID | PR65/19-22430 | es |
dc.relation.projectID | BARM-RILO-18-02 | es |
dc.relation.projectID | FIS2017-88410-P | es |
dc.relation.projectID | FIS2017-88410-P | es |
dc.relation.projectID | FQM160 | es |
dc.relation.projectID | SOMM17/6105/UGR | es |
dc.relation.projectID | A07 | es |
dc.relation.projectID | 2020/37/N/ST2/01751 | es |
dc.relation.projectID | DIR WK/2017/05 | es |
dc.relation.projectID | 839481 | es |
dc.relation.publisherversion | https://dx.doi.org/10.1103/PhysRevC.105.025502 | es |
dc.identifier.doi | 10.1103/PhysRevC.105.025502 | es |
dc.journaltitle | Physical Review C | es |
dc.publication.volumen | 105 | es |
dc.publication.issue | 2 | es |
dc.publication.initialPage | 025502 | es |
dc.contributor.funder | United States Department of Energy (DOE) | es |
dc.contributor.funder | Universidad Complutense de Madrid | es |
dc.contributor.funder | University of Turin | es |
dc.contributor.funder | Ministerio de Economía y Competitividad (MINECO). España | es |
dc.contributor.funder | European Commission | es |
dc.contributor.funder | Junta de Andalucia | es |
dc.contributor.funder | University of Tokyo | es |
dc.contributor.funder | NCN Preludium | es |
dc.contributor.funder | Ministry of Science and Higher Education, Poland | es |
dc.contributor.funder | SKA South Africa | es |