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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...
| Autores principales: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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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 |
| _version_ | 1780976781845594112 |
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| author | Agafonova, N. Alexandrov, A. Anokhina, A. Aoki, S. Ariga, A. Ariga, T. Bertolin, A. Bozza, C. Brugnera, R. Buontempo, S. Chernyavskiy, M. Chukanov, A. Consiglio, L. D'Ambrosio, N. De Lellis, G. De Serio, M. del Amo Sanchez, P. Di Crescenzo, A. Di Ferdinando, D. Di Marco, N. Dmitrievsky, S. Dracos, M. Duchesneau, D. Dusini, S. Dzhatdoev, T. Ebert, J. Ereditato, A. Fini, R.A. Fukuda, T. Galati, G. Garfagnini, A. Gentile, V. Goldberg, J. Gorbunov, S. Gornushkin, Y. Grella, G. Guler, A.M. Gustavino, C. Hagner, C. Hara, T. Hayakawa, T. Hollnagel, A. Ishiguro, K. Iuliano, A. Jakovčić, K. Jollet, C. Kamiscioglu, C. Kamiscioglu, M. Kim, S.H. Kitagawa, N. Kliček, B. Kodama, K. Komatsu, M. Kose, U. Kreslo, I. Laudisio, F. Lauria, A. Longhin, A. Loverre, P. Malgin, A. Mandrioli, G. Matsuo, T. Matveev, V. Mauri, N. Medinaceli, E. Meregaglia, A. Mikado, S. Miyanishi, M. Mizutani, F. Monacelli, P. Montesi, M.C. Morishima, K. Muciaccia, M.T. Naganawa, N. Naka, T. Nakamura, M. Nakano, T. Niwa, K. Ogawa, S. Okateva, N. Ozaki, K. Paoloni, A. Paparella, L. Park, B.D. Pasqualini, L. Pastore, A. Patrizii, L. Pessard, H. Podgrudkov, D. Polukhina, N. Pozzato, M. Pupilli, F. Rodak, M. Roganova, T. Rokujo, H. Rosa, G. Ryazhskaya, O. Sato, O. Schembri, A. Shakiryanova, I. Shchedrina, T. Shibayama, E. Shibuya, H. Shiraishi, T. Simone, S. Sirignano, C. Sirri, G. Sotnikov, A. Spinetti, M. Stanco, L. Starkov, N. Stellacci, S.M. Stipčević, M. Strolin, P. Takahashi, S. Tenti, M. Terranova, F. Tioukov, V. Tufanli, S. Vasina, S. Vilain, P. Voevodina, E. Votano, L. Vuilleumier, J.L. Wilquet, G. Yoon, C.S. |
| author_facet | Agafonova, N. Alexandrov, A. Anokhina, A. Aoki, S. Ariga, A. Ariga, T. Bertolin, A. Bozza, C. Brugnera, R. Buontempo, S. Chernyavskiy, M. Chukanov, A. Consiglio, L. D'Ambrosio, N. De Lellis, G. De Serio, M. del Amo Sanchez, P. Di Crescenzo, A. Di Ferdinando, D. Di Marco, N. Dmitrievsky, S. Dracos, M. Duchesneau, D. Dusini, S. Dzhatdoev, T. Ebert, J. Ereditato, A. Fini, R.A. Fukuda, T. Galati, G. Garfagnini, A. Gentile, V. Goldberg, J. Gorbunov, S. Gornushkin, Y. Grella, G. Guler, A.M. Gustavino, C. Hagner, C. Hara, T. Hayakawa, T. Hollnagel, A. Ishiguro, K. Iuliano, A. Jakovčić, K. Jollet, C. Kamiscioglu, C. Kamiscioglu, M. Kim, S.H. Kitagawa, N. Kliček, B. Kodama, K. Komatsu, M. Kose, U. Kreslo, I. Laudisio, F. Lauria, A. Longhin, A. Loverre, P. Malgin, A. Mandrioli, G. Matsuo, T. Matveev, V. Mauri, N. Medinaceli, E. Meregaglia, A. Mikado, S. Miyanishi, M. Mizutani, F. Monacelli, P. Montesi, M.C. Morishima, K. Muciaccia, M.T. Naganawa, N. Naka, T. Nakamura, M. Nakano, T. Niwa, K. Ogawa, S. Okateva, N. Ozaki, K. Paoloni, A. Paparella, L. Park, B.D. Pasqualini, L. Pastore, A. Patrizii, L. Pessard, H. Podgrudkov, D. Polukhina, N. Pozzato, M. Pupilli, F. Rodak, M. Roganova, T. Rokujo, H. Rosa, G. Ryazhskaya, O. Sato, O. Schembri, A. Shakiryanova, I. Shchedrina, T. Shibayama, E. Shibuya, H. Shiraishi, T. Simone, S. Sirignano, C. Sirri, G. Sotnikov, A. Spinetti, M. Stanco, L. Starkov, N. Stellacci, S.M. Stipčević, M. Strolin, P. Takahashi, S. Tenti, M. Terranova, F. Tioukov, V. Tufanli, S. Vasina, S. Vilain, P. Voevodina, E. Votano, L. Vuilleumier, J.L. Wilquet, G. Yoon, C.S. |
| author_sort | Agafonova, N. |
| collection | CERN |
| description | 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 |$\Delta m^2_{41} \sim {0.3}\, {\rm eV}^{2}$|. |
| id | cern-2847477 |
| institution | Organización Europea para la Investigación Nuclear |
| language | eng |
| publishDate | 2022 |
| record_format | invenio |
| spelling | cern-28474772023-07-24T03:09:11Zdoi:10.1093/ptep/ptad012http://cds.cern.ch/record/2847477engAgafonova, N.Alexandrov, A.Anokhina, A.Aoki, S.Ariga, A.Ariga, T.Bertolin, A.Bozza, C.Brugnera, R.Buontempo, S.Chernyavskiy, M.Chukanov, A.Consiglio, L.D'Ambrosio, N.De Lellis, G.De Serio, M.del Amo Sanchez, P.Di Crescenzo, A.Di Ferdinando, D.Di Marco, N.Dmitrievsky, S.Dracos, M.Duchesneau, D.Dusini, S.Dzhatdoev, T.Ebert, J.Ereditato, A.Fini, R.A.Fukuda, T.Galati, G.Garfagnini, A.Gentile, V.Goldberg, J.Gorbunov, S.Gornushkin, Y.Grella, G.Guler, A.M.Gustavino, C.Hagner, C.Hara, T.Hayakawa, T.Hollnagel, A.Ishiguro, K.Iuliano, A.Jakovčić, K.Jollet, C.Kamiscioglu, C.Kamiscioglu, M.Kim, S.H.Kitagawa, N.Kliček, B.Kodama, K.Komatsu, M.Kose, U.Kreslo, I.Laudisio, F.Lauria, A.Longhin, A.Loverre, P.Malgin, A.Mandrioli, G.Matsuo, T.Matveev, V.Mauri, N.Medinaceli, E.Meregaglia, A.Mikado, S.Miyanishi, M.Mizutani, F.Monacelli, P.Montesi, M.C.Morishima, K.Muciaccia, M.T.Naganawa, N.Naka, T.Nakamura, M.Nakano, T.Niwa, K.Ogawa, S.Okateva, N.Ozaki, K.Paoloni, A.Paparella, L.Park, B.D.Pasqualini, L.Pastore, A.Patrizii, L.Pessard, H.Podgrudkov, D.Polukhina, N.Pozzato, M.Pupilli, F.Rodak, M.Roganova, T.Rokujo, H.Rosa, G.Ryazhskaya, O.Sato, O.Schembri, A.Shakiryanova, I.Shchedrina, T.Shibayama, E.Shibuya, H.Shiraishi, T.Simone, S.Sirignano, C.Sirri, G.Sotnikov, A.Spinetti, M.Stanco, L.Starkov, N.Stellacci, S.M.Stipčević, M.Strolin, P.Takahashi, S.Tenti, M.Terranova, F.Tioukov, V.Tufanli, S.Vasina, S.Vilain, P.Voevodina, E.Votano, L.Vuilleumier, J.L.Wilquet, G.Yoon, C.S.Updated constraints on sterile neutrino mixing in the OPERA experiment using a new $\nu_e$ identification methodhep-exParticle Physics - ExperimentThis 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 |$\Delta m^2_{41} \sim {0.3}\, {\rm eV}^{2}$|.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 $\Delta m^2_{41} \sim 0.3\,\mathrm{eV}^2$.arXiv:2211.04636oai:cds.cern.ch:28474772022-11-08 |
| spellingShingle | hep-ex Particle Physics - Experiment Agafonova, N. Alexandrov, A. Anokhina, A. Aoki, S. Ariga, A. Ariga, T. Bertolin, A. Bozza, C. Brugnera, R. Buontempo, S. Chernyavskiy, M. Chukanov, A. Consiglio, L. D'Ambrosio, N. De Lellis, G. De Serio, M. del Amo Sanchez, P. Di Crescenzo, A. Di Ferdinando, D. Di Marco, N. Dmitrievsky, S. Dracos, M. Duchesneau, D. Dusini, S. Dzhatdoev, T. Ebert, J. Ereditato, A. Fini, R.A. Fukuda, T. Galati, G. Garfagnini, A. Gentile, V. Goldberg, J. Gorbunov, S. Gornushkin, Y. Grella, G. Guler, A.M. Gustavino, C. Hagner, C. Hara, T. Hayakawa, T. Hollnagel, A. Ishiguro, K. Iuliano, A. Jakovčić, K. Jollet, C. Kamiscioglu, C. Kamiscioglu, M. Kim, S.H. Kitagawa, N. Kliček, B. Kodama, K. Komatsu, M. Kose, U. Kreslo, I. Laudisio, F. Lauria, A. Longhin, A. Loverre, P. Malgin, A. Mandrioli, G. Matsuo, T. Matveev, V. Mauri, N. Medinaceli, E. Meregaglia, A. Mikado, S. Miyanishi, M. Mizutani, F. Monacelli, P. Montesi, M.C. Morishima, K. Muciaccia, M.T. Naganawa, N. Naka, T. Nakamura, M. Nakano, T. Niwa, K. Ogawa, S. Okateva, N. Ozaki, K. Paoloni, A. Paparella, L. Park, B.D. Pasqualini, L. Pastore, A. Patrizii, L. Pessard, H. Podgrudkov, D. Polukhina, N. Pozzato, M. Pupilli, F. Rodak, M. Roganova, T. Rokujo, H. Rosa, G. Ryazhskaya, O. Sato, O. Schembri, A. Shakiryanova, I. Shchedrina, T. Shibayama, E. Shibuya, H. Shiraishi, T. Simone, S. Sirignano, C. Sirri, G. Sotnikov, A. Spinetti, M. Stanco, L. Starkov, N. Stellacci, S.M. Stipčević, M. Strolin, P. Takahashi, S. Tenti, M. Terranova, F. Tioukov, V. Tufanli, S. Vasina, S. Vilain, P. Voevodina, E. Votano, L. Vuilleumier, J.L. Wilquet, G. Yoon, C.S. Updated constraints on sterile neutrino mixing in the OPERA experiment using a new $\nu_e$ identification method |
| title | Updated constraints on sterile neutrino mixing in the OPERA experiment using a new $\nu_e$ identification method |
| title_full | Updated constraints on sterile neutrino mixing in the OPERA experiment using a new $\nu_e$ identification method |
| title_fullStr | Updated constraints on sterile neutrino mixing in the OPERA experiment using a new $\nu_e$ identification method |
| title_full_unstemmed | Updated constraints on sterile neutrino mixing in the OPERA experiment using a new $\nu_e$ identification method |
| title_short | Updated constraints on sterile neutrino mixing in the OPERA experiment using a new $\nu_e$ identification method |
| title_sort | updated constraints on sterile neutrino mixing in the opera experiment using a new $\nu_e$ identification method |
| topic | hep-ex Particle Physics - Experiment |
| url | https://dx.doi.org/10.1093/ptep/ptad012 http://cds.cern.ch/record/2847477 |
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