Nucleon binding energy and transverse momentum imbalance in neutrino-nucleus reactions

dc.contributor.affiliationPontificia Universidad Católica del Perú. Departamento de Ciencias
dc.contributor.authorCai, T.
dc.contributor.authorLu, X.-G.
dc.contributor.authorHarewood, L.A.
dc.contributor.authorWret, C.
dc.contributor.authorAkbar, F.
dc.contributor.authorAndrade, D.A.
dc.contributor.authorAscencio-Sosa, M.V.
dc.contributor.authorBellantoni, L.
dc.contributor.authorBercellie, A.
dc.contributor.authorBetancourt, M.
dc.contributor.authorBodek, A.
dc.contributor.authorBonilla, J.L.
dc.contributor.authorBravar, A.
dc.contributor.authorBudd, H.
dc.contributor.authorCaceres, G.
dc.contributor.authorCarneiro, M.F.
dc.contributor.authorCoplowe, D.
dc.contributor.authorda Motta, H.
dc.contributor.authorDar, Z.A.
dc.date.accessioned2026-03-13T17:00:13Z
dc.date.issued2020
dc.description.abstractWe have measured new observables based on the final state kinematic imbalances in the mesonless production of ${\ensuremath{\nu}}_{\ensuremath{\mu}}+A\ensuremath{\rightarrow}{\ensuremath{\mu}}^{\ensuremath{-}}+p+X$ in the MINER\ensuremath{\nu}A tracker. Components of the muon-proton momentum imbalances parallel ($\ensuremath{\delta}{p}_{\mathrm{Ty}}$) and perpendicular ($\ensuremath{\delta}{p}_{\mathrm{Tx}}$) to the momentum transfer in the transverse plane are found to be sensitive to the nuclear effects such as Fermi motion, binding energy, and non-quasielastic (QE) contributions. The QE peak location in $\ensuremath{\delta}{p}_{\mathrm{Ty}}$ is particularly sensitive to the binding energy. Differential cross sections are compared to predictions from different neutrino interaction models. The Fermi gas models presented in this study cannot simultaneously describe features such as QE peak location, width, and the non-QE events contributing to the signal process. Correcting the genie's binding energy implementation according to theory causes better agreement with data. Hints of proton left-right asymmetry are observed in $\ensuremath{\delta}{p}_{\mathrm{Tx}}$. Better modeling of the binding energy can reduce the bias in neutrino energy reconstruction, and these observables can be applied in current and future experiments to better constrain nuclear effects.
dc.description.sponsorshipFunding: This work was supported by the Fermi National Accelerator Laboratory under US Department of Energy Contract No. DE-AC02-07CH11359, which included the MINER\u03BDA construction project. Construction support was also granted by the United States National Science Foundation under Grant No. PHY-0619727 and by the University of Rochester. Support for participating scientists was provided by NSF and DOE (USA), by CAPES and CNPq (Brazil), by CoNaCyT (Mexico), by Proyecto Basal FB 0821, CONICYT PIA ACT1413, Fondecyt 3170845 and 11130133 (Chile), by DGI-PUCP and UDI/VRI-IGI-UNI (Peru), by the Latin American Center for Physics (CLAF), by Science and Technology Facilities Council (UK), and by NCN Opus Grant No. 2016/21/B/ST2/01092 (Poland). We thank the MINOS Collaboration for use of its near detector data. We acknowledge the dedicated work of the Fermilab staff responsible for the operation and maintenance of the beam line and detector and the Fermilab Computing Division for support of data processing.
dc.identifier.doihttps://doi.org/10.1103/PhysRevD.101.092001
dc.identifier.urihttp://hdl.handle.net/20.500.14657/206542
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.ispartofurn:issn:2470-0010
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.sourcePhysical Review D; Vol. 101, Núm. 9 (2020)
dc.subjectPhysics
dc.subjectNeutrino
dc.subjectMuon
dc.subjectNuclear physics
dc.subjectNucleon
dc.subjectParticle physics
dc.subjectObservable
dc.subjectFermi Gamma-ray Space Telescope
dc.subjectEnergy (signal processing)
dc.subjectProton
dc.subjectAsymmetry
dc.subjectBinding energy
dc.subjectAtomic physics
dc.subjectQuantum mechanics
dc.subject.ocdehttps://purl.org/pe-repo/ocde/ford#1.03.03
dc.titleNucleon binding energy and transverse momentum imbalance in neutrino-nucleus reactions
dc.typehttp://purl.org/coar/resource_type/c_6501
dc.type.otherArtículo
dc.type.versionhttps://vocabularies.coar-repositories.org/version_types/c_970fb48d4fbd8a85/

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