Proton Transparency and Neutrino Physics: New Methods and Modeling
S. Dytman, M. Betancourt, N. Steinberg, L.B. Weinstein, A. Ashkenazi, J. Tena-Vidal, A. Papadopoulou, G. Chambers-Wall, J. Smith, P. Achenbach, J. S. Alvarado, M.J. Amaryan, H. Atac, L. Baashen, N.A. Baltzell, L. Barion, M. Bashkanov, M. Battaglieri, F. Benmokhtar, A. Bianconi

TL;DR
This paper introduces a new data-driven method to measure proton transparency in electron-nucleus scattering, highlighting discrepancies in current simulation models like GENIE, which are crucial for neutrino physics experiments.
Contribution
The study presents a novel measurement technique for proton transparency using electron scattering data and demonstrates the need for improved modeling in neutrino interaction simulations.
Findings
Measured proton transparency across helium, carbon, and iron targets.
Identified deficiencies in GENIE's description of nuclear ground state and rescattering.
Results support refining simulation models for better neutrino experiment accuracy.
Abstract
Extracting accurate results from neutrino oscillation and cross section experiments requires accurate simulation of the neutrino-nucleus interaction. The rescattering of outgoing hadrons (final state interactions) by the rest of the nucleus is an important component of these interactions. We present a new measurement of proton transparency (defined as the fraction of outgoing protons that emerge without significant rescattering) using electron-nucleus scattering data recorded by the CLAS detector at Jefferson Laboratory on helium, carbon, and iron targets. This analysis by the Electrons for Neutrinos () collaboration uses a new data-driven method to extract the transparency. It defines transparency as the ratio of electron-scattering events with a detected proton to quasi-elastic electron-scattering events where a proton should have been knocked out. Our results are consistent…
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Taxonomy
TopicsNeutrino Physics Research · Particle physics theoretical and experimental studies · Dark Matter and Cosmic Phenomena
