Materias dentro de su búsqueda.
Materias dentro de su búsqueda.
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2561por Stolarczyk, T“…This report presents 10 years of research concerning the neutrino through the experiments Gallex, Nomad and Antares to which the has contributed. …”
Publicado 2003
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2562“…A data analysis procedure is proposed for a tau neutrino appearance experiment in which the Cherenkov light from tau leptons created in neutrino-nucleon interactions is imaged using an HPD-based RICH counter. …”
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2563
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2564“…A complete simulation of the SPS neutrino beam line at CERN showed significant variations in the intensity and composition of the neutrino beam when FLUKA standalone instead of the GEANT-FLUKA package is used to simulate particle production in the Be target.…”
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2565
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2566
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2567
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2568
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2569por Machado, M V T“…The ultrahigh energy neutrino-nucleon cross sections are computed taking into account different phenomenological implementations of the non-linear QCD dynamic s. …”
Publicado 2003
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2570
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2571
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2572por Tonazzo, A“…The main R&D items toward construction of a Neutrino Factory are presented, with emphasis on a Muon Ionization Cooling Experiment.…”
Publicado 2004
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2573por Önengüt, G, Van Dantzig, R, De Jong, M, Oldeman, R G C, Güler, M, Köse, U, Tolun, P, Catanesi, M G, Muciaccia, M T, Winter, Klaus, Van de Vyver, B, Vilain, P, Wilquet, G, Saitta, B, Di Capua, E, Ogawa, S, Shibuya, H, Goldberg, J, Hristova, I R, Kawamura, T, Kolev, D, Kayis-Topaksu, A, Meinhard, H, Panman, J, Rozanov, A, Tsenov, R V, Zucchelli, P, Uiterwijk, J W E, Chikawa, M, Song, J S, Yoon, C S, Kodama, K, Ushida, N, Hara, T, Aoki, S, Delbar, T, Favart, D, Grégoire, G, Kalinin, S, Makhlyoueva, I V, Bruski, N, Frekers, D, Tsukerman, I, Shamanov, V V, Khovanskii, V D, Gorbunov, P, Artamonov, A V, Sato, Y, Tezuka, I, Barbuto, E, Bozza, C, Grella, G, Romano, G, Sirignano, C, Sorrentino, S, Dore, U, Loverre, P F, Ludovici, L, Rosa, G, Santacesaria, R, Satta, A, Spada, F R, Okusawa, T, Hoshino, K, Kawada, J, Komatsu, M, Miyanishi, M, Nakamura, M, Nakano, T, Narita, K, Niu, K, Niwa, K, Nonaka, N, Sato, O, Toshito, T, Buontempo, S, Cocco, A G, D'Ambrosio, N, De Lellis, G, De Rosa, G, Di Capua, F, Fiorillo, G, Marotta, A, Messina, M, Migliozzi, P, Scotto-Lavina, L, Strolin, P, Tioukov, V“…During the years 1994-97, the emulsion target of the CHORUS detector was exposed to the wide-band neutrino beam of the CERN SPS of 27 GeV average neutrino energy. …”
Publicado 2005
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2574por Vives, Oscar“…In this model, we obtain exactly maximal atmospheric mixing, large although not maximal solar mixing and a normal neutrino hierarchy. All neutrino parameters are basically fixed. …”
Publicado 2005
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2575
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2576
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2577
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2578
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2579
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2580