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1761
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1762
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1763
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1764
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1765“…The neutrino physics program at the LHC, which will soon be initiated by the FASER experiment, will provide unique opportunities for precision studies of neutrino interaction vertices at high energies. …”
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1766
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1767por 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“…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. …”
Publicado 2021
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1768por Franckowiak, Anna“…However, cosmic rays produce gamma-ray photons and neutrinos in interactions with matter and photon fields in or close to their source. …”
Publicado 2021
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1769por De Serio, Marilisa“…Among hidden particles, the search for Heavy Neutral Leptons is very strongly motivated by theory, as they would explain simultaneously the baryon asymmetry of the Universe and the observed neutrino masses. The expected copious production of Ds mesons at the beam dump, producing tau neutrinos through fully leptonic decays, makes SHiP also ideal to study tau neutrino physics with unprecedented sensitivity. …”
Publicado 2021
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1770
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1771
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1772
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1773por Novak, Tadej“…Multiple theories beyond the Standard Model predict the existence of heavy neutrinos, such as the Type I or Type III seesaw mechanisms that can explain the light neutrino masses, or left-right symmetric models that restore parity symmetry in weak interactions at a higher energy scale and predict right-handed counterparts to the weak gauge bosons. …”
Publicado 2022
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1774
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1775“…The discovery that neutrinos have mass has important consequences for cosmology. …”
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1776por Berryman, Jeffrey M., Blinov, Nikita, Brdar, Vedran, Brinckmann, Thejs, Bustamante, Mauricio, Cyr-Racine, Francis-Yan, Das, Anirban, de Gouvêa, André, Denton, Peter B., Dev, P.S. Bhupal, Dutta, Bhaskar, Esteban, Ivan, Fiorillo, Damiano F.G., Gerbino, Martina, Ghosh, Subhajit, Ghosh, Tathagata, Grohs, Evan, Han, Tao, Hannestad, Steen, Hostert, Matheus, Huber, Patrick, Hyde, Jeffrey, Kelly, Kevin J., Kling, Felix, Liu, Zhen, Lattanzi, Massimiliano, Loverde, Marilena, Pandey, Sujata, Saviano, Ninetta, Sen, Manibrata, Shoemaker, Ian M., Tangarife, Walter, Zhang, Yongchao, Zhang, Yue“…Neutrinos are the Standard Model (SM) particles which we understand the least, often due to how weakly they interact with the other SM particles. …”
Publicado 2022
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1777por Alekou, A., Baussan, E., Kraljevic, N. Blaskovic, Blennow, M., Bogomilov, M., Bouquerel, E., Burgman, A., Carlile, C.J., Cederkall, J., Christiansen, P., Collins, M., Morales, E. Cristaldo, Cupial, P., Alessi, L.D., Danared, H., de Andre, J.P.A.M., Delahaye, J.P., Dracos, M., Efthymiopoulos, I., Ekelof, T., Eshraqi, M., Fanourakis, G., Fernandez-Martinez, E., Folsom, B., Gazis, N., Geralis, Th., Ghosh, M., Gokbulut, G., Halic, L., Topaksu, A. Kayis, Kildetoft, B., Klicek, B., Koziol, M., Krhac, K., Lacny, L., Lindroos, M., Mezzetto, M., Oglakci, M., Ohlsson, T., Olvegard, M., Ota, T., Park, J., Patrzalek, D., Petkov, G., Poussot, P., Johansson, R., Rosauro-Alcaraz, S., Szybinski, B., Snamina, J., Stavropoulos, G., Stipcevic, M., Terranova, F., Thomas, J., Tolba, T., Trachanas, E., Tsenov, R., Vankova-Kirilova, G., Vassilopoulos, N., Wildner, E., Wurtz, J., Zormpa, O., Zou, Y.“…A high power target station facility will be needed to produce a well-focused intense (super) mu-neutrino beam. The physics performance of that neutrino Super Beam in conjunction with a megaton underground Water Cherenkov neutrino far detector installed at a distance of either 360 km or 540 km from the ESS, the baseline, has been evaluated.…”
Publicado 2022
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1778por Pastore, A“…The beam dump will be a copious source of hidden particles, together with active neutrinos of all flavours. The SHiP detector is designed to detect feebly interacting particles and to perform precision studies of neutrino and anti-neutrino interactions, too. …”
Publicado 2020
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1779por Physicists, Team“…Discoveries: The 3 neutrinos Theory: Why and how do the neutrinos oscillate? …”
Publicado 2022
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1780