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2941
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2942
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2943“…We analyze the possible observable consequences of R-parity violating transitions in large-volume neutrino telescopes.…”
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2944“…We propose an experiment to test the hypothesis that the reported anomaly on atmospheric neutrino fluxes is due to nu_mu <-> nu_x oscillations. …”
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2945
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2946
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2947por Hampel, W, Heusser, G, Kiko, J, Kirsten, T, Laubenstein, M, Pernicka, E, Rau, W, Rönn, U, Wójcik, M, Von Ammon, R, Ebert, K H, Fritsch, T, Heidt, D, Henrich, E, Stieglitz, L, Weirich, F, Balata, M, Sann, M, Hartmann, F X, Bellotti, E, Cattadori, c, Cremonesi, O, Ferrari, N, Fiorini, Ettore, Zanotti, L, Altmann, M, Von Feilitzsch, F, Mössbauer, R L, Berthomieu, G, Schatzman, E L, Carmi, I, Dostrovsky, I, Bacci, Cesare, Belli, P, Bernabei, R, D'Angelo, S, Paoluzi, L, Bevilacqua, A, Cribier, Michel, Gosset, L G, Rich, J, Spiro, Michel, Tao, Charling, Vignaud, D, Boger, J, Hahn, R L, Rowley, J K, Stönner, R W, Weneser, JEnlace del recurso
Publicado 1998
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2948por Vilain, P, Wilquet, G, Beyer, R, Flegel, Wilfried, Mouthuy, T, Øverås, H, Panman, J, Rozanov, A N, Winter, Klaus, Zacek, G, Zacek, V, Büsser, F W, Foos, C, Gerland, L, Layda, T, Niebergall, F, Rädel, G, Stähelin, P, Voss, T, Lemaître, V, Favart, D, Grégoire, G, Knoops, E, Gorbunov, P, Grigoriev, E A, Khovanskii, V D, Maslennikov, A M, Lippich, W, Nathaniel, A, Staude, A, Vogt, J, Cocco, A G, Ereditato, A, Fiorillo, G, Marchetti-Stasi, F, Palladino, Vittorio, Strolin, P, Capone, A, De Pedis, D, Dore, U, Frenkel-Rambaldi, A, Loverre, P F, Macina, Daniela, Piredda, G, Santacesaria, R, Di Capua, E, Ricciardi, S, Saitta, B, Akkus, B, Arik, E, Serin-Zeyrek, M, Sever, R, Tolun, P, Hiller, K, Nahnhauer, R, Roloff, H E“…The results of a leading-order QCD analysis of neutrino-induced charm production are presented. They are based on a sample of 4111 $\numu$- and 871 $\anumu$-induced opposite-sign dimuon events with $E_{\mu 1},E_{\mu 2} > 6~{\rm GeV}$, $35 < E_{\nu} < 290~{\rm GeV}$ and $Q^2> 5.5\,{\rm GeV^2}$, observed in the CHARM~II detector exposed to the CERN wideband neutrino and antineutrino beams. …”
Publicado 1998
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2949
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2950“…We present an overview of the future projects concerning the neutrino oscillation physics in Europe. Recently a joint CERN-LNGS scientific committee has reviewed several proposals both for the study of atmospheric neutrinos and for long (LBL) and short baseline (SBL) neutrino oscillation experiments. …”
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2951por Anassontzis, E G, Barone, M, Fahrun, E, Foudas, C, Gialas, G, Grammatikakis, George A, Katsanevas, S, Kourkoumelis, C, Manousakis-Katsikakis, A, Odian, A C, Resvanis, L K, Siotis, I, Sotiriou, S A, Voulgaris, G, Ball, A E, Cartacci, A M, Dell'Agnello, L, Monteleoni, B, Naumov, V A, Perrone, L, Martini, A, Nicoletti, G, Trasatti, L, Valente, V, Keusen, U, Koske, P, Rathlev, J, Voigt, G, Curti, F, De Marchis, G, Piccari, L, Ameli, F, Bonori, M, Bosio, C, Bottai, S, Capone, A, Desiati, P, Massa, F, Rikalin, V, Valente, E, Bezrukov, L B, Butkevich, A V, Dedenko, L G, Karaevsky, S K, Mironovich, A A, Zakharov, L M, Zheleznykh, I M, Zhukov, V, Demidova, T A, Deyneko, A, Eremeev, A P, Paka, V T, Permyakov, A A, Platonov, M N, Rucol, V K, Surin, N N, Sheremet, N A, Albul, V I, Ledenev, V VEnlace del recurso
Publicado 1998
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2952por Schubert, Klaus R“…Neutrino oscillations with three lepton families are described with a unitary mixing matrix U in analogy to the quark mixing matrix V(CKM). …”
Publicado 1999
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2953
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2954por Aglietta, M, Bologna, G, Bonesini, M, Calvi, M, Castellina, A, Curioni, A, Ferrari, P, Fulgione, W, Ghia, P L, Kokoulin, R P, Mannocchi, G, Murtas, F, Murtas, G P, Negri, P, Paganoni, M, Periale, L, Petrukhin, A A, Picchi, P, Pullia, Antonio, Ragazzi, S, Redaelli, N G, Satta, L, Tabarelli de Fatis, T, Terranova, F, Tonazzo, A, Trinchero, G C, Vallania, P, Villone, BEnlace del recurso
Publicado 1998
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2955por Adelberger, E.G., Ortiz, C., Garcia, A., Swanson, H.E., Beck, M., Tengblad, O., Borge, M.J.G., Martel, I., Bichsel, H.“…The positron-neutrino correlation in the $0^+ \to 0^+ \beta$ decay of $^{32}$Ar was measured at ISOLDE by analyzing the effect of lepton recoil on the shape of the narrow proton group following the superallowed decay. …”
Publicado 1999
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2956“…The vacuum oscillation (VO) solution to the solar anomaly requires an extremely small neutrino mass splitting, Delta m^2_{sol}\leq 10^{-10} eV^2. …”
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2957“…We discuss the special class of models where nearly maximal neutrino mixing is produced through the see-saw mechanism, starting from only nearly diagonal matrices for charged leptons, Dirac neutrinos and Majorana right-handed neutrinos.…”
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2958
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2959por CERN PhotoLab“…Ricci working on a magnet : this proton beam will hit a target and generate pions (neutrino parents) to be focussed by the "neutrino horn".…”
Publicado 1963
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2960“…We derive the general renormalization group equations for these physical parameters and apply them to study the impact of radiative effects on neutrino physics. In particular, we examine the existing solutions to the solar and atmospheric neutrino problems, derive conclusions on their theoretical naturalness, and show how some of the measured neutrino parameters could be determined by purely radiative effects. …”
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