Updated constraints on sterile neutrino mixing in the OPERA experiment using a new \(\nu_e\) identification method
This paper describes a new \(\nu_e\) identification method specifically designed to improve the low-energy (\(< 30\,\mathrm{GeV}\)) \(\nu_e\) identification efficiency attained by enlarging the emulsion film scanning volume with the next generation emulsion readout system. A relative increase of...
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Veröffentlicht in: | arXiv.org 2023-01 |
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Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | This paper describes a new \(\nu_e\) identification method specifically designed to improve the low-energy (\(< 30\,\mathrm{GeV}\)) \(\nu_e\) 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 \(\nu_e\) 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 \(\nu_e\) candidate is found. The analysis combined with the \(\nu_\tau\) appearance results improves the upper limit on \(\sin^2 2\theta_{\mu e}\) to 0.016 at 90% C.L. in the MiniBooNE allowed region \(\Delta m^2_{41} \sim 0.3\,\mathrm{eV}^2\). |
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ISSN: | 2331-8422 |