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Materias dentro de su búsqueda.
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2141“…This requires the computation of a migration matrix $M_{ij}$ which describes the contributions of the tau neutrinos of a given energy $E_i$, to the muon neutrinos of an apparent energy $E_j$. …”
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2142“…We present an extension of the Standard Model (SM) based on the discrete flavor symmetry S3 which gives a neutrino mass matrix with two-zero texture of Fritzsch-type and nearly diagonal charged lepton mass matrix. …”
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2143“…Finally we combine these results with the information on neutrino mass differences and mixing from the global analysis of neutrino oscillation experiments and derive the presently allowed ranges for the two laboratory probes o f the absolute scale of neutrino mass: the effective electron neutrino mass in single beta decay and the effective Majorana neutrino mass in neutrinoless $\beta\beta$ decay.…”
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2144“…This consists of the Minimal Supersymmetric Standard Model with the addition of massive right handed Majorana neutrinos and their supersymmetric partners, and where the seesaw mechanism is used for the lightest neutrino mass generation. …”
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2145
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2146“…We investigate how models for neutrino-nucleus cross sections based on different assumptions for the nuclear dynamics affect the forecasted sensitivities to neutrino oscillation parameters at future neutrino facilities. …”
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2147“…We discuss the design of the muon capture front end of the neutrino factory International Design Study. In the front end, a proton bunch on a target creates secondary pions that drift into a capture transport channel, decaying into muons. …”
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2148por Efthymiopoulos, I, Cornelis, K, Gschwendtner, E, Pardons, A, Vincke, H, Wenninger, JMaterias: “…3: NEU2012: Structuring the accelerator neutrino community…”
Publicado 2012
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2149por Jonker, M, Udo, Fred, Allaby, James V, Amaldi, Ugo, Barbiellini, Guido, Flegel, Wilfried, Kozanecki, Witold, Mess, K H, Metcalf, M, Meyer, J, Monacelli, P, Orr, R S, Panman, J, Wetherell, Alan M, Winter, Klaus, Blobel, Volker, Büsser, F W, Gall, P D, Grote, H, Kröger, B J, Metz, E, Niebergall, F, Ranitzsch, K H, Stähelin, P, Gorbunov, P, Grigoriev, E A, Kaftanov, V S, Khovanskii, V D, Rosanov, A, Baroncelli, A, Biancastelli, Roberto, Borgia, B, Bosio, C, Capone, A, Ferroni, F, Longo, E, De Notaristefani, F, Pistilli, P, Santoni, C, Valente, VEnlace del recurso
Publicado 1982
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2150
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2151
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2152por Holder, M, Knobloch, J, May, J, Paar, H P, Palazzi, P, Ranjard, F, Schlatter, W D, Steinberger, Jack, Suter, H, Wahl, H, Whitaker, S, Williams, E G H, Eisele, Franz, Kleinknecht, K, Lierl, H, Spahn, G, Willutzki, H J, Dorth, W, Dydak, Friedrich, Geweniger, C, Hepp, V, Tittel, K, Wotschack, J, Bloch, P, Devaux, B, Maillard, J, Peyaud, B, Rander, J, Savoy-Navarro, Aurore, Turlay, René, Navarria, Francesco LuigiEnlace del recurso
Publicado 1977
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2153
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2154por Holder, M, Knobloch, J, May, J, Paar, H P, Palazzi, P, Ranjard, F, Schlatter, W D, Steinberger, Jack, Suter, H, Wahl, H, Whitaker, S, Williams, E G H, Eisele, Franz, Geweniger, C, Kleinknecht, K, Spahn, G, Willutzki, H J, Dorth, W, Dydak, Friedrich, Hepp, V, Tittel, K, Wotschack, J, Bloch, P, Devaux, B, Grimm, M, Maillard, J, Peyaud, B, Rander, J, Savoy-Navarro, Aurore, Turlay, René, Navarria, Francesco LuigiEnlace del recurso
Publicado 1978
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2155por Agafonova, N., Aleksandrov, A., Altinok, O., Anokhina, A., Aoki, S., Ariga, A., Ariga, T., Autiero, D., Badertscher, A., Bagulya, A., Bendhabi, A., Bertolin, A., Bozza, C., Brugiere, T., Brugnera, R., Brunet, F., Brunetti, G., Buontempo, S., Cazes, A., Chaussard, L., Chernyavsky, M., Chiarella, V., Chukanov, A., D'Ambrosio, N., Dal Corso, F., De Lellis, G., del Amo Sanchez, P., Declais, Y., De Serio, M., Di Capua, F., Di Crescenzo, A., Di Ferdinando, D., Di Marco, N., Dmitrievski, S., Dracos, M., Duchesneau, D., Dusini, S., Dzhatdoev, T., Ebert, J., Egorov, O., Enikeev, R., Ereditato, A., Esposito, L.S., Favier, J., Ferber, T., Fini, R.A., Frekers, D., Fukuda, T., Garfagnini, A., Giacomelli, G., Giorgini, M., Gollnitz, C., Goldberg, J., Golubkov, D., Goncharova, L., Gornushkin, Y., Grella, G., Grianti, F., Guler, A.M., Gustavino, C., Hagner, C., Hamada, K., Hara, T., Hierholzer, M., Hollnagel, A., Hoshino, K., Ieva, M., Ishida, H., Jakovcic, K., Jollet, C., Juget, F., Kamiscioglu, M., Kazuyama, K., Kim, S.H., Kimura, M., Kitagawa, N., Klicek, B., Knuesel, J., Kodama, K., Komatsu, M., Kose, U., Kreslo, I., Kubota, H., Lazzaro, C., Lenkeit, J., Lippi, I., Ljubicic, A., Longhin, A., Loverre, P., Lutter, G., Malgin, A., Mandrioli, G., Mannai, K., Marteau, J., Matsuo, T., Matveev, V., Mauri, N., Medinaceli, E., Meisel, F., Meregaglia, A., Migliozzi, P., Mikado, S., Miyamoto, S., Monacelli, P., Morishima, K., Moser, U., Muciaccia, M.T., Naganawa, N., Naka, T., Nakamura, M., Nakano, T., Naumov, D., Nikitina, V., Niwa, K., Nonoyama, Y., Ogawa, S., Okateva, N., Olchevski, A., Paniccia, M., Paoloni, A., Park, B.D., Park, I.G., Pastore, A., Patrizii, L., Pennacchio, E., Pessard, H., Pretzl, K., Pilipenko, V., Pistillo, C., Polukhina, N., Pozzato, M., Pupilli, F., Rescigno, R., Roganova, T., Rokujo, H., Romano, G., Rosa, G., Rostovtseva, I., Rubbia, A., Russo, A., Ryasny, V., Ryazhskaya, O., Sato, O., Sato, Y., Schembri, A., Schmidt-Parzefall, W., Schroeder, H., Scotto Lavina, L., Sheshukov, A., Shibuya, H., Shoziyoev, G., Simone, S., Sioli, M., Sirignano, C., Sirri, G., Song, J.S., Spinetti, M., Stanco, L., Starkov, N., Stipcevic, M., Strauss, T., Strolin, P., Takahashi, S., Tenti, M., Terranova, F., Tezuka, I., Tioukov, V., Tolun, P., Trabelsi, A., Tran, T., Tufanli, S., Vilain, P., Vladimirov, M., Votano, L., Vuilleumier, J.L., Wilquet, G., Wonsak, B., Yakushev, V., Yoon, C.S., Yoshioka, T., Yoshida, J., Zaitsev, Y., Zemskova, S., Zghiche, A., Zimmermann, R.“…OPERA collected muon-neutrino interactions during the 2008 and 2009 physics runs of the CNGS neutrino beam, produced at CERN with an energy range of about 5-35 GeV. …”
Publicado 2011
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2156por Hansl-Kozanecka, Traudl, Holder, M, Knobloch, J, May, J, Paar, H P, Hansl, T, Palazzi, P, Para, A, Ranjard, F, Schlatter, W D, Steinberger, Jack, Suter, H, von Rüden, Wolfgang, Wahl, H, Whitaker, S, Williams, E G H, Eisele, Franz, Kleinknecht, K, Lierl, H, Spahn, G, Willutzki, H J, Dorth, W, Dydak, Friedrich, Geweniger, C, Hepp, V, Tittel, K, Wotschack, J, Bloch, P, Devaux, B, Loucatos, Sotirios S, Maillard, J, Peyaud, B, Rander, J, Savoy-Navarro, Aurore, Turlay, René, Navarria, Francesco LuigiEnlace del recurso
Publicado 1978
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2157
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2158
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2159por De Groot, J G H, Hansl-Kozanecka, Traudl, Holder, M, Knobloch, J, May, J, Paar, H P, Palazzi, P, Para, A, Ranjard, F, Schlatter, W D, Steinberger, Jack, Suter, H, von Rüden, Wolfgang, Wahl, H, Whitaker, S, Williams, E G H, Eisele, Franz, Kleinknecht, K, Lierl, H, Spahn, G, Willutzki, H J, Dorth, W, Dydak, Friedrich, Geweniger, C, Hepp, V, Tittel, K, Wotschack, J, Bloch, P, Devaux, B, Loucatos, Sotirios S, Maillard, J, Peyaud, B, Rander, J, Savoy-Navarro, Aurore, Turlay, René, Navarria, Francesco LuigiEnlace del recurso
Publicado 1978
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2160por Pozzato, Michele“…The OPERA experiment aims at the direct observation of ν_mu -> ν_tau oscillations in the CNGS (CERN Neutrinos to Gran Sasso) neutrino beam produced at CERN; since the ν_e contamination in the CNGS beam is low, OPERA will also be able to study the sub-dominant oscillation channel ν_mu -> ν_e. …”
Publicado 2009
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