Electron-induced single-pion production to constrain the neutron structure in $^{40}$Ar. A proof of concept
J. García-Marcos, M. Hooft, T. Franco-Munoz, N. Jachowicz, J. M. Udías, K. Niewczas, A. Nikolakopoulos, R. González-Jiménez
TL;DR
The paper investigates electron-induced single-pion production on $^{40}$Ar via a triple-coincidence reaction $^{40}$Ar$(e,e'p\pi^-)$ as a method to constrain the neutron spectral function in argon, aiming to reduce systematic uncertainties in neutrino experiments using argon detectors. A RPWIA framework with an IPSM ground state and a Ghent-Hybrid single-pion production model is combined with a NuWro intranuclear cascade to predict signal and backgrounds, under kinematics that emphasize $E_m$ and $p_m$ regions tied to the neutron shell structure. Feasibility is shown to be facility-dependent: MAMI's high-resolution, small-acceptance spectrometers can resolve neutron-shell peaks in $E_m$ with $E_m<70$ MeV and $p_m<350$ MeV, while CLAS's large acceptance yields larger cross sections but cannot resolve shell structure due to its energy resolution. The work provides a proof-of-concept that such triple-coincidence measurements can illuminate neutron structure in $^{40}$Ar and inform neutrino-nucleus interaction modeling, with next steps including final-state distortions and uncertainty quantification.
Abstract
We study electron-induced single-pion production as a way to constrain the neutron structure of $^{40}$Ar, information that is necessary for neutrino experiments using argon detectors. The proposed experimental signal consists in detecting in coincidence the scattered electron, a proton and a $π^-$. We performed simulations compatible with the experimental conditions of the MAMI (University of Mainz) and CLAS (Jefferson Lab) facilities. We have computed cross sections and evaluated the main backgrounds. MAMI is a three-spectrometer system with extremely good energy resolution and small acceptances. We found that, by choosing specific values of the final particle's momenta, the shell structure can be well resolved, with negligible background contributions. CLAS is a large solid angle detector with poorer energy resolution. In both cases, the background can be kept under control by performing cuts in missing energy and missing momentum; however, in CLAS, the shell structure cannot be resolved due to the energy resolution. We conclude that MAMI is particularly appropriate for the proposed experiment, whereas CLAS is better suited for other studies.
