Materias dentro de su búsqueda.
Materias dentro de su búsqueda.
-
3501“…This volume offers a valuable insight into various aspects of the ongoing work directed at measuring neutrino mass. It took twenty years to refute the assertions of Bethe and Peierls that neutrinos were not observable, but it has since been realised that much can be learnt from these particles. …”
Enlace del recurso
-
3502“…A proposal for a new system to capture signals in the Optical Module (OM) of an underwater neutrino telescope is described. It concentrates on the problem of power consumption and time precision. …”
Enlace del recurso
Enlace del recurso
-
3503
-
3504
-
3505
-
3506por Lyubushkin, V, Popov, B, Kim, J J, Camilleri, L, Levy, J M, Mezzetto, M, Naumov, D, Alekhin, S, Astier, P, Autiero, D, Baldisseri, A, Baldo-Ceolin, M, Banner, M, Bassompierre, G, Benslama, K, Besson, N, Bird, I, Blumenfeld, B, Bobisut, F, Bouchez, J, Boyd, S, Bueno, A, Bunyatov, S, Cardini, A, Cattaneo, P W, Cavasinni, V, Cervera-Villanueva, A, Challis, R, Chukanov, A, Collazuol, G, Conforto, G, Conta, C, Contalbrigo, M, Cousins, R, Daniels, D, Degaudenzi, H, Del Prete, T, De Santo, A, Dignan, T, Di Lella, L, do Couto e Silva, E, Dumarchez, J, Ellis, M, Feldman, G J, Ferrari, R, Ferrre, D, Flaminio, V, Fraternali, M, Gaillard, J M, Gangler, E, Geiser, A, Geppert, D, Gibin, D, Gninenko, S, Godley, A, Gomez-Cadenas, J J, Gosset, J, Gling, C, Gouanre, M, Grant, A, Graziani, G, Guglielmi, A, Hagner, C, Hernando, J, Hubbard, D, Hurst, P, Hyett, N, Iacopini, E, Joseph, C, Juget, F, Kent, N, Kirsanov, M, Klimov, O, Kokkonen, J, Kovzelev, A, Krasnoperov, A, Kulagin, S, Kustov, D, Lacaprara, S, Lachaud, C, Lakic, B, Lanza, A, La Rotonda, L, Laveder, M, Letessier-Selvon, A, Ling, J, Linssen, L, Ljubicic, A, Long, J, Lupi, A, Marchionni, A, Martelli, F, Mchain, X, Mendiburu, J P, Meyer, J P, Mishra, S R, Moorhead, G F, Ndlec, P, Nefedov, Yu, Nguyen-Mau, C, Orestano, D, Pastore, F, Peak, L S, Pennacchio, E, Pessard, H, Placci, A, Polesello, G, Pollmann, D, Polyarush, A, Poulsen, C, Rebuffi, L, Rico, J, Riemann, P, Roda, C, Rubbia, A, Salvatore, F, Samoylov, O, Schahmaneche, K, Schmidt, B, Schmidt, T, Sconza, A, Seaton, M, Sevior, M, Sillou, D, Soler, F J P, Sozzi, G, Steele, D, Stiegler, U, Stipcevic, M, Stolarczyk, Th, Tareb-Reyes, M, Taylor, G N, Tereshchenko, V, Toropin, A, Touchard, A M, Tovey, S N, Tran, M T, Tsesmelis, E, Ulrichs, J, Vacavant, L, Valdata-Nappi, M, Valuev, V, Vannucci, F, Varvell, K E, Veltri, M, Vercesi, V, Vidal-Sitjes, G, Vieira, J M, Vinogradova, T, Weber, F V, Weisse, T, Wilson, F F, Winton, L J, Wu, Q, Yabsley, B D, Zaccone, H, Zuber, K, Zuccon, P“…We have studied the muon neutrino and antineutrino quasi-elastic (QEL) scattering reactions ($\nu_\mu n\to \mu^- p$ and $\bar{\nu}_\mu p\to \mu^+ n$) using a set of experimental data collected by the NOMAD collaboration. …”
Publicado 2008
Enlace del recurso
Enlace del recurso
-
3507“…We suggest a R-parity violation in the right-handed neutrino sector. The violation is suppressed by a see-saw mechanism. …”
Enlace del recurso
Enlace del recurso
-
3508por Kirsanov, M“…The left-right symmetric model can explain the origin of parity violation in weak interactions and predicts the existence of additional $W_R$ and $Z'$ gauge bosons and heavy right-handed neutrino states $N_l$. $N_l$ can be partners of light neutrino states ($l=e,\mu,\tau$), related to their non-zero masses through the see-saw mechanism. …”
Publicado 2009
Enlace del recurso
-
3509
-
3510
-
3511
-
3512
-
3513
-
3514
-
3515
-
3516por Abgrall, Nicolas“…Among other goals, the NA61-SHINE (SPS Heavy Ion and Neutrino Experiment) experiment at the CERN SPS aims at precision measurements (5% and below) for both neutrino and cosmic ray experiments: those will improve the prediction of the neutrino flux for the T2K experiment at J-PARC and the prediction of muon production in the propagation of air showers for the Auger experiment. …”
Publicado 2010
Enlace del recurso
-
3517“…We investigate supersymmetric scenarios in which neutrino masses are generated by effective d=6 operators in the Kahler potential, rather than by the standard d=5 superpotential operator. …”
Enlace del recurso
Enlace del recurso
info:eu-repo/semantics/article -
3518“…We investigate the possible solution to these inconsistencies with non standard neutrino interactions, assuming that they come as extra contributions to the $\nu_{\alpha}\nu_{\beta}$ and $\nu_{\alpha}e$ vertices that affect both the propagation of neutrinos in the sun and their detection. …”
Enlace del recurso
info:eu-repo/semantics/article -
3519
-
3520