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Updated constraints on sterile neutrino mixing in the OPERA experiment using a new $\nu_e$ identification method
This paper describes a new ν_e identification method specifically designed to improve the low-energy (|$\lt {30}\, {\rm GeV}$|) ν_e identification efficiency attained by enlarging the emulsion film scanning volume with the next-generation emulsion readout system. A relative increase of 25–70% in t...
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Lenguaje: | eng |
Publicado: |
2022
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1093/ptep/ptad012 http://cds.cern.ch/record/2847477 |
Sumario: | This paper describes a new ν_e identification method specifically designed to improve the low-energy (|$\lt {30}\, {\rm GeV}$|) ν_e identification efficiency attained by enlarging the emulsion film scanning volume with the next-generation emulsion readout system. A relative increase of 25–70% in the ν_e low-energy region is expected, leading to improvements in the OPERA sensitivity to neutrino oscillations in the framework of the 3 + 1 model. The method is applied to a subset of data where the detection efficiency increase is expected to be more relevant, and one additional ν_e candidate is found. The analysis combined with the ν_τ appearance results improves the upper limit on sin ^22θμe to 0.016 at 90% C.L. in the MiniBooNE allowed region |$\Delta m^2_{41} \sim {0.3}\, {\rm eV}^{2}$|. |
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