-
3421por Popa, V“…We present the results of the measurements performed in the occasion of the 2001 total solar eclipse, looking for visible photons emitted through a possible radiative decay of solar neutrinos. We establish lower limits for the \nu_2 and \nu_3 proper lifetimes above 10^3 s/eV, for neutrino masses larger than 10^{-2} eV.…”
Publicado 2004
Enlace del recurso
Enlace del recurso
-
3422
-
3423
-
3424por Johnson, G“…The experiment also confirms that neutrinos, long thought to be weightless, have a tiny bit of mass. …”
Publicado 2002
Enlace del recurso
-
3425por Munro, M“…Work at the Sudbury Neutrino Observatory in Ontario, Canada, is being hailed as one of the top breakthroughs of the year by both the journal Science and the American Institute of Physics (1 page).…”
Publicado 2002
Enlace del recurso
-
3426por Zei, Riccardo“…Bose-Einstein Correlations in one and two dimensions have been studied in charged current muon-neutrino interaction events collected with NOMAD. In one dimension the Bose-Einstein effect has been analyzed with the Goldhaber and the Kopylov parametrizations. …”
Publicado 2004
Enlace del recurso
-
3427
-
3428“…Motivated by the Super-Kamiokande data, we revisit models with U(1) symmetries and discuss the origin of neutrino masses and mixings in such theories. We show that, in models with just three light neutrinos and a hierarchy of neutrino masses, large (2-3) mixing fixes the lepton doublet U(1) charges and is thus related to the structure of the charged lepton mass matrix. …”
Enlace del recurso
Enlace del recurso
-
3429
-
3430por Migliozzi, P“…In this paper we review the next possible steps that can be done for neutrino oscillation experiments with accelerators…”
Publicado 2003
Enlace del recurso
-
3431“…We discuss a particularly symmetric model of neutrino mixings where, with good accuracy, the atmospheric mixing angle theta_{23} is maximal, theta_{13}=0 and the solar angle satisfies sin^2(theta_{12})=1/3 (Harrison-Perkins-Scott (HRS) matrix). …”
Enlace del recurso
Enlace del recurso
-
3432
-
3433
-
3434
-
3435“…We calculate the running of low-energy neutrino parameters from the bottom up, parameterizing the unknown seesaw parameters in terms of the dominance matrix $R$. …”
Enlace del recurso
Enlace del recurso
-
3436por Aguilar, J A, Albert,A, Amram, P, Anghinolfi, M, Anton, G, Anvar, S, Ardellier-Desages, F E, Aslanides, E, Aubert, Jean-Jacques, Azoulay, R, Bailey, D, Basa, S, Battaglieri, M, Becherini, Y, Bellotti, R, Beltramelli, J, Bertin, V, Billault, M, Blaes, R, Blanc, F, Bland, R W, De Botton, N R, Boulesteix, J, Bouwhuis, M C, Brooks, C B, Bradbury, S M, Bruijn, R, Brunner, J, Bugeon, F, Burgio, G F, Cafagna, F, Calzas, A, Caponetto, L, Carmona, E, Carr, J, Cartwright, S L, Cecchini, S, Charvis, P, Circella, M, Colnard, C, Compère, C, Croquette, J, Cooper, S, Coyle, P, Cuneo, S, Damy, G, Van Dantzig, R, Deschamps, A, De Marzo, C, Destelle, J J, Vita, R De, Dinkelspiler, B, Dispau, G, Drougou, J F, Druillole, F, Engelen, J, Favard, S, Feinstein, F, Ferry, S, Festy, D, Fopma, J, Fuda, J L, Gallone, J M, Giacomelli, G, Girard, N, Goret, P, Gournay, J F, Hallewell, G D, Hartmann, B, Heijboer, A, Hello, Y, Hernàndez-Rey, J J, Herrouin, G, Hössle, J, Hoffmann, C, Hubbard, John R, Jaquet, M, Jong, M de, Jouvenot, F, Kappes, A, Karg, T, Karka, S, Karola, M, Katz, U, Keller, P, Kooijman, P, Korolkova, E V, Kouchner, A, Kretschmer, W, Kudryavtsev, V A, Lafoux, H, Lagier, P, Lamare, P, Languillat, J C, Laubier, L, Legou, T, Guen, Y Le, Le Provost, H, Van Suu, Le, Nigro, L Lo, Presti, D Lo, Loucatos, Sotirios S, Louis, F, Lyashuk, V, Magnier, P, Marcelin, M, Margiotta, A, Maron, C, Massol, A, Mazéas, F, Mazeau, B, Mazure, A, McMillan, J E, Michel, J L, Millot, C, Milovanovic, A, Montanet, François, Montaruli, T, Morel, J P, Moscoso, L, Nezri, E, Niess, V, Nooren, G J, Ogden, P, Olivetto, C, Palanque-Delabrouille, Nathalie, Payre, P, Petta, C, Pineau, J P, Poinsignon, J, Popa, V, Potheau, R, Pradier, T, Racca, C, Randazzo, N, Real, D, Van Rens, B A P, Réthoré, F, Ripani, M, Roca-Blay, V, Romeyer, A, Rollin, J F, Romita, M, Rose, H J, Rostovtsev, A, Ruppi, M, Russo, G V, Sacquin, Yu, Saouter, S, Schuller, J P, Schuster, W, Sokalski, I A, Suvorova, O, Spooner, N J C, Spurio, M, Stolarczyk, T, Stubert, D, Taiuti, M, Thompson, L F, Tilav, S, Usik, A, Valdy, P, Vallage, B, Vaudaine, G, Vernin, P, Virieux, J, Vladimirsky, E, Vries, G de, De Witt-Huberts, P K A, De Wolf, E, Zaborov, D, Zaccone, Henri, Zakharov, V, Zavatarelli, S, De Zornoza, J D, Zúñiga, JEnlace del recurso
Publicado 2004
-
3437
-
3438
-
3439“…We analyze the effects of lepton asymmetry on neutrino oscillations and on cosmological nucleosynthesis (CN) with oscillating neutrinos. …”
Enlace del recurso
Enlace del recurso
-
3440por Akama, K“…The author proposes sum rules which can be used for testing the scaling hypothesis and its powerlike breakdown in deep inelastic neutrino scattering. These sum rules are written in terms of the mean values of quantities determined solely by the outgoing leptons. …”
Publicado 1975
Enlace del recurso
Enlace del recurso