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OPERA tau neutrino charged current interactions
The OPERA experiment was designed to discover the v$_\tau$ appearance in a v$_\mu$ beam, due to neutrino oscillations. The detector, located in the underground Gran Sasso Laboratory, consisted of a nuclear photographic emulsion/lead target with a mass of about 1.25 kt, complemented by electronic det...
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| Lenguaje: | eng |
| Publicado: |
2021
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1038/s41597-021-00991-y http://cds.cern.ch/record/2783198 |
| _version_ | 1780972039684751360 |
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| author | Agafonova, N Alexandrov, A Anokhina, A Aoki, S Ariga, A Ariga, T Bertolin, A Bozza, C Brugnera, R Buonaura, A 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 Fornari, F 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 Lavasa, 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 Park, B D Pasqualini, L Pastore, A Patrizii, L Pessard, H Podgrudkov, D Polukhina, N Pozzato, M Pupilli, F Roda, M Roganova, T Rokujo, H Rosa, G Ryazhskaya, O Sato, O Shakirianova, I Schembri, A Shchedrina, T Shibayama, E Shibuya, H Shiraishi, T Šimko, 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 Tsanaktsidis, I Tufanli, S Ustyuzhanin, A Vasina, S García, M Vidal 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 Buonaura, A 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 Fornari, F 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 Lavasa, 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 Park, B D Pasqualini, L Pastore, A Patrizii, L Pessard, H Podgrudkov, D Polukhina, N Pozzato, M Pupilli, F Roda, M Roganova, T Rokujo, H Rosa, G Ryazhskaya, O Sato, O Shakirianova, I Schembri, A Shchedrina, T Shibayama, E Shibuya, H Shiraishi, T Šimko, 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 Tsanaktsidis, I Tufanli, S Ustyuzhanin, A Vasina, S García, M Vidal Vilain, P Voevodina, E Votano, L Vuilleumier, J L Wilquet, G Yoon, C S |
| author_sort | Agafonova, N |
| collection | CERN |
| description | The OPERA experiment was designed to discover the v$_\tau$ appearance in a v$_\mu$ beam, due to neutrino oscillations. The detector, located in the underground Gran Sasso Laboratory, consisted of a nuclear photographic emulsion/lead target with a mass of about 1.25 kt, complemented by electronic detectors. It was exposed from 2008 to 2012 to the CNGS beam: an almost pure vμ beam with a baseline of 730 km, collecting a total of 1.8·10$^{20}$ protons on target. The OPERA Collaboration eventually assessed the discovery of v$_\mu \to$ v$_\tau$ oscillations with a statistical significance of 6.1 $\sigma$ by observing ten v$_\tau$ CC interaction candidates. These events have been published on the Open Data Portal at CERN. This paper provides a detailed description of the v$_\tau data sample to make it usable by the whole community. |
| id | cern-2783198 |
| institution | Organización Europea para la Investigación Nuclear |
| language | eng |
| publishDate | 2021 |
| record_format | invenio |
| spelling | cern-27831982021-10-05T19:11:58Zdoi:10.1038/s41597-021-00991-yhttp://cds.cern.ch/record/2783198engAgafonova, NAlexandrov, AAnokhina, AAoki, SAriga, AAriga, TBertolin, ABozza, CBrugnera, RBuonaura, ABuontempo, SChernyavskiy, MChukanov, AConsiglio, LD'Ambrosio, NDe Lellis, GDe Serio, Mdel Amo Sanchez, PDi Crescenzo, ADi Ferdinando, DDi Marco, NDmitrievsky, SDracos, MDuchesneau, DDusini, SDzhatdoev, TEbert, JEreditato, AFini, R AFornari, FFukuda, TGalati, GGarfagnini, AGentile, VGoldberg, JGorbunov, SGornushkin, YGrella, GGuler, A MGustavino, CHagner, CHara, THayakawa, THollnagel, AIshiguro, KIuliano, AJakovčić, KJollet, CKamiscioglu, CKamiscioglu, MKim, S HKitagawa, NKliček, BKodama, KKomatsu, MKose, UKreslo, ILaudisio, FLauria, ALavasa, ALonghin, ALoverre, PMalgin, AMandrioli, GMatsuo, TMatveev, VMauri, NMedinaceli, EMeregaglia, AMikado, SMiyanishi, MMizutani, FMonacelli, PMontesi, M CMorishima, KMuciaccia, M TNaganawa, NNaka, TNakamura, MNakano, TNiwa, KOgawa, SOkateva, NOzaki, KPaoloni, APark, B DPasqualini, LPastore, APatrizii, LPessard, HPodgrudkov, DPolukhina, NPozzato, MPupilli, FRoda, MRoganova, TRokujo, HRosa, GRyazhskaya, OSato, OShakirianova, ISchembri, AShchedrina, TShibayama, EShibuya, HShiraishi, TŠimko, TSimone, SSirignano, CSirri, GSotnikov, ASpinetti, MStanco, LStarkov, NStellacci, S MStipčević, MStrolin, PTakahashi, STenti, MTerranova, FTioukov, VTsanaktsidis, ITufanli, SUstyuzhanin, AVasina, SGarcía, M VidalVilain, PVoevodina, EVotano, LVuilleumier, J LWilquet, GYoon, C SOPERA tau neutrino charged current interactionsParticle Physics - ExperimentThe OPERA experiment was designed to discover the v$_\tau$ appearance in a v$_\mu$ beam, due to neutrino oscillations. The detector, located in the underground Gran Sasso Laboratory, consisted of a nuclear photographic emulsion/lead target with a mass of about 1.25 kt, complemented by electronic detectors. It was exposed from 2008 to 2012 to the CNGS beam: an almost pure vμ beam with a baseline of 730 km, collecting a total of 1.8·10$^{20}$ protons on target. The OPERA Collaboration eventually assessed the discovery of v$_\mu \to$ v$_\tau$ oscillations with a statistical significance of 6.1 $\sigma$ by observing ten v$_\tau$ CC interaction candidates. These events have been published on the Open Data Portal at CERN. This paper provides a detailed description of the v$_\tau data sample to make it usable by the whole community.oai:cds.cern.ch:27831982021 |
| spellingShingle | Particle Physics - Experiment Agafonova, N Alexandrov, A Anokhina, A Aoki, S Ariga, A Ariga, T Bertolin, A Bozza, C Brugnera, R Buonaura, A 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 Fornari, F 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 Lavasa, 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 Park, B D Pasqualini, L Pastore, A Patrizii, L Pessard, H Podgrudkov, D Polukhina, N Pozzato, M Pupilli, F Roda, M Roganova, T Rokujo, H Rosa, G Ryazhskaya, O Sato, O Shakirianova, I Schembri, A Shchedrina, T Shibayama, E Shibuya, H Shiraishi, T Šimko, 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 Tsanaktsidis, I Tufanli, S Ustyuzhanin, A Vasina, S García, M Vidal Vilain, P Voevodina, E Votano, L Vuilleumier, J L Wilquet, G Yoon, C S OPERA tau neutrino charged current interactions |
| title | OPERA tau neutrino charged current interactions |
| title_full | OPERA tau neutrino charged current interactions |
| title_fullStr | OPERA tau neutrino charged current interactions |
| title_full_unstemmed | OPERA tau neutrino charged current interactions |
| title_short | OPERA tau neutrino charged current interactions |
| title_sort | opera tau neutrino charged current interactions |
| topic | Particle Physics - Experiment |
| url | https://dx.doi.org/10.1038/s41597-021-00991-y http://cds.cern.ch/record/2783198 |
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