Search for Neutrino-Induced Neutral-Current Δ Radiative Decay in MicroBooNE and a First Test of the MiniBooNE Low Energy Excess under a Single-Photon Hypothesis
Metadatos
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American Physical Society
Fecha
2022-03-14Referencia bibliográfica
Abratenko, P., An, R., Anthony, J., Arellano, L., Asaadi, J., Ashkenazi, A., ... & Smith, A. (2022). Search for Neutrino-Induced Neutral-Current Δ Radiative Decay in MicroBooNE and a First Test of the MiniBooNE Low Energy Excess under a Single-Photon Hypothesis. Physical review letters, 128(11), 111801. [https://doi.org/10.1103/PhysRevLett.128.111801]
Patrocinador
European Union’s Horizon 2020 Marie Skłodowska-Curie Actions; Fermi Research Alliance, LLC DE-AC02-07CH11359; High Energy Physics and Nuclear Physics; United Kingdom Research and Innovation; National Science Foundation; U.S. Department of Energy; Office of Science; Science and Technology Facilities Council; Royal Society; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungResumen
We report results from a search for neutrino-induced neutral current (NC) resonant Δð1232Þ baryon
production followed by Δ radiative decay, with a h0.8i GeV neutrino beam. Data corresponding to
MicroBooNE’s first three years of operations (6.80 × 1020 protons on target) are used to select single-photon
events with one or zero protons and without charged leptons in the final state (1γ1p and 1γ0p, respectively).
The background is constrained via an in situ high-purity measurement of NC π0 events, made possible via
dedicated 2γ1p and 2γ0p selections. A total of 16 and 153 events are observed for the 1γ1p and 1γ0p
selections, respectively, compared to a constrained background prediction of 20.5 3.65ðsystÞ and 145.1
13.8ðsystÞ events. The data lead to a bound on an anomalous enhancement of the normalization of NC Δ
radiative decay of less than 2.3 times the predicted nominal rate for this process at the 90% confidence level
(C.L.). The measurement disfavors a candidate photon interpretation of the MiniBooNE low-energy excess as
a factor of 3.18 times the nominal NC Δ radiative decay rate at the 94.8% C.L., in favor of the nominal
prediction, and represents a greater than 50-fold improvement over the world’s best limit on single-photon
production in NC interactions in the sub-GeV neutrino energy range.