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Neutrino-induced one-pion production revisited: The νμn→μ−nπ+ channel

Understanding single pion production reactions on free nucleons is the first step towards a correct description of these processes in nuclei, which are important for signal and background contributions in current and near future accelerator neutrino oscillation experiments. In this work, we reanalyz...

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Bibliographic Details
Published in:Physical review. D 2017-03, Vol.95 (5), p.053007
Main Authors: Hernández, E, Nieves, J
Format: Article
Language:English
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Summary:Understanding single pion production reactions on free nucleons is the first step towards a correct description of these processes in nuclei, which are important for signal and background contributions in current and near future accelerator neutrino oscillation experiments. In this work, we reanalyze our previous studies of neutrino-induced one-pion production on nucleons for outgoing πN invariant masses below 1.4 GeV. Our motivation is to get a better description of the νμn→μ−nπ+ cross section, for which current theoretical models give values significantly below data. This channel is very sensitive to the crossed Δ(1232) contribution and thus, to spin 1/2 components in the Rarita-Schwinger Δ propagator. We show how these spin 1/2 components are nonpropagating and give rise to contact interactions. In this context, we point out that the discrepancy with experiment might be corrected by the addition of appropriate extra contact terms and argue that this procedure will provide a natural solution to the νμn→μ−nπ+ puzzle. To keep our model simple, in this work, we propose to change the strength of the spin 1/2 components in the Δ propagator and use the νμn→μ−nπ+ data to constraint its value. With this modification, we now find a good reproduction of the νμn→μ−nπ+ cross section without affecting the good results previously obtained for the other channels. We also explore how this change in the Δ propagator affects our predictions for pion photoproduction and find also a better agreement with experiment than with the previous model.
ISSN:2470-0010
2470-0029
DOI:10.1103/PhysRevD.95.053007