Origin of the low-mass electron pair excess in light nucleus-nucleus collisions
The HADES Collaboration: G. Agakishiev, A. Balanda, D. Belver, A. V., Belyaev, A. Blanco, M. B\"ohmer, J. L. Boyard, P. Braun-Munzinger, P., Cabanelas, E. Castro, S. Chernenko, T. Christ, M. Destefanis, J. D\'iaz, F., Dohrmann, A. Dybczak, L. Fabbietti, O. V. Fateev

TL;DR
This study measures electron pair production in elementary and light nucleus collisions, revealing a significant excess in neutron-proton reactions and suggesting current models do not fully explain the production mechanisms.
Contribution
First measurement of electron pairs in n+p reactions at 1.25 GeV/u, highlighting differences from p+p and implications for modeling light nucleus collisions.
Findings
Electron pair yield in n+p is ten times higher than in p+p for invariant mass > 0.15 GeV/c2.
Electron spectra in C+C are consistent with a superposition of elementary n+p and p+p reactions.
Current models do not fully account for the observed electron pair production mechanisms.
Abstract
We report measurements of electron pair production in elementary p+p and d+p reactions at 1.25 GeV/u with the HADES spectrometer. For the first time, the electron pairs were reconstructed for n+p reactions by detecting the proton spectator from the deuteron breakup. We find that the yield of electron pairs with invariant mass Me+e- > 0.15 GeV/c2 is about an order of magnitude larger in n+p reactions as compared to p+p. A comparison to model calculations demonstrates that the production mechanism is not sufficiently described yet. The electron pair spectra measured in C+C reactions are compatible with a superposition of elementary n+p and p+p collisions, leaving little room for additional electron pair sources in such light collision systems.
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