First Measurement of the Superscaling Variable as a Function of Visible Kinematics in Charged-Current Quasi-Elastic Neutrino--Nucleus Scattering
The MINERvA Collaboration, L. Giannessi, S. Akhter, Z. Ahmad Dar, N. S. Alex, M. Sajjad Athar, J. Felix, L. Fields, R. Gran, E. Granados, D. A. Harris, A. Klustová, M. Kordosky, D. Last, and A. Lozano, S. Manly, W. A. Mann, K. S. McFarland, M. Mehmood, O. Moreno, J. G. Morfín, J. K. Nelson, G. N. Perdue, C. Pernas, M. A. Ramírez, R. D. Ransome, N. Roy, D. Ruterbories, F. Sánchez, H. Schellman, C. J. Solano Salinas, D. S. Correia, V. S. Syrotenko, N. H. Vaughan, A. V. Waldron, L. Zazueta
Abstract
We report the first measurement of the superscaling variable ψ vis in neutrino--nucleus scattering, using charged-current quasielastic-like νμ-Carbon interactions collected by the MINERvA experiment in the medium-energy NuMI beam. Originally developed to characterize phenomena of scaling with respect to atomic number and momentum transfer in quasielastic electron-nucleus scattering, ψ is reconstructed here from visible final-state kinematics (ψ vis). ψ vis is used here as an externally calibrated variable whose peak position is sensitive to the invisible nuclear missing energy. We measure ψ vis as functions of the hadronic recoil ΣTp and muon transverse momentum pTμ, comparing background-subtracted data to five neutrino--nucleus interaction models via a forward-folding technique. The predicted ψ vis diverges most strongly among model predictions at low ΣTp and pTμ, where agreement with data is also poorest, exposing which models fail to capture the phase-space dependence of the missing energy and therefore the neutrino energy as extrapolated from visible kinematics. Among tested models, we find that the Relativistic Mean Field approach predicts more accurately the ψ vis peak position.
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