Results 41 to 50 of about 189,461 (221)
Progress in neutrino oscillation searches and their implications
, 2003 Neutrino Oscillation, in which a given flavour of neutrino transforms into
another is a powerful tool for probing small neutrino masses. The intrinsic
neutrino properties involved are neutrino mass squared difference $\Delta m^2$
and the mixing angle in ...A Bandyopadhyay, A Bandyopadhyay, B T Cleveland, C Athanassopoulos, Ch Berger, Ch. Berger, D Buskulic, D Casper, E A Hawker, E Fiorini, F Terranova, G L Fogli, H Ejiri, H V Klapdor-Kleingrothaus, J N Abdurashitov, J N Bahcall, L Borodovsky, L Wolfenstein, M Agiletta, M Altmann, M Goodman, M Honda, M Maltoni, Q R Ahmad, R Becker-Szendy, S Choubey, S Choubey, S H Ahn, S M Bilenky, S M Bilenky, S P Mikheyev, S T Petcov, S T Petcov, Srubabati Goswami, T K Gaisser, V D Barger, V Paolone, W Hampel, Y Farzan, Y Fukuda, Y Fukuda, Y Fukuda +41 morecore +1 more sourceStatus of the solutions to neutrino anomalies based on non-standard
neutrino interactions
, 2000 We review the status of the solutions to neutrino anomalies by
flavor-changing as well as flavor-diagonal neutrino interactions. While it is
difficult to explain the atmospheric neutrino data the solar neutrino data can
be well accounted for by the ...Aulakh, Bahcall, Bahcall, Barbieri, Barger, Becker-Szendy, Bergman, Bergmann, Bergmann, Bergmann, Ellis, Fogli, Fogli, Foot, Fornengo, Frampton, Fukugita, Geer, Geer, Gonzalez-Garcia, Gribov, Guzzo, Hall, Hiroshi Nunokawa, Johnson, Lipari, Mikheyev, Pisano, Ross, Roulet, Valle, Wolfenstein, Wolfenstein, Zwirner +33 morecore +1 more sourceSolar Neutrinos Before and After Neutrino 2004 [PDF]
, 2004 We compare, using a three neutrino analysis, the allowed neutrino oscillation
parameters and solar neutrino fluxes determined by the experimental data
available Before and After Neutrino 2004. New data available after Neutrino2004
include refined KamLAND Bahcall, John N., Gonzalez-Garcia, M. C., Pena-Garay, Carlos +2 morecore +4 more sourcesStandard Solar Neutrinos [PDF]
, 1996 An improved standard solar model has been used to calculate the fluxes of
standard solar neutrinos. It includes premain sequence evolution, element
diffusion, partial ionization effects, and all the possible nuclear reactions
between the main elements ...Anders, Anselmann, Arnon Dar, Bahcall, Bahcall, Bahcall, Barker, Caughlan, Christensen-Dalsgaard, Cleveland, Dar, Dar, Dawarakanath, Dzitko, Filippone, Geiss, Giora Shaviv, Greife, Grevesse, Grevesse, Grevesse, Hata, Hata, Hernandez, Hilgemeier, Johnson, Kamionkowski, Kavanagh, Kim, Kovetz, Krauss, Krawinkel, Langanke, Mikheyev, Motobayashi, Osborne, Parke, Parker, Parker, Parker, Rogers, Shaviv, Shaviv, Sturenburg, Vaughn, Volk, Wolfenstein, Wolfenstein +47 morecore +2 more sourcesMajorana neutrino masses and neutrino oscillations [PDF]
Physical Review D, 2001 We examine some patterns of Majorana neutrino mass matrix which is compatible with the phenomenological lepton flavor mixing matrix and non-observation of neutrinoless double beta decay. Imposing $(M_ν)_{ee}=0$ for the Majorana neutrino mass matrix in the leading order, we obtain a relationship between the solar mixing angle and the neutrino masses ...Kang, Sin Kyu, Kim, C. S.openaire +2 more sourcesNeutrino mass matrix with U(2) flavor symmetry and neutrino oscillations
, 1997 The three neutrino mass matrices in the $SU(5)\times U(2)$ model are studied
focusing on the neutrino oscillation experiments. The atmospheric neutrino
anomaly could be explained by the large $\nu_{\mu} - \nu_{\tau}$ oscillation.A. Pomarol, B. Achkar, C. Athanassopoulos, C. Athanassopoulos, C. Athanassopoulos, C. D. Carone, G. Fiorentini, J. E. Hill, K. Winter, L. Borodovsky, L. Wolfenstein, L. Wolfenstein, M. Dine, Morimitsu Tanimoto, N. Hata, P. H. Frampton, P. H. Frampton, P. I. Krastev, P. I. Krastev, P. Pouliot, R. Barbieri, R. Barbieri, R. Barbieri, R. M. Barnett, S. Ahlen, S. P. Mikheyev, S. Wojcicki, W. W. M. Allison, Y. Fukuda +28 morecore +1 more sourceEvidence for muon neutrino oscillation in an accelerator-based
experiment [PDF]
, 2004 We present results for muon neutrino oscillation in the KEK to Kamioka (K2K)
long-baseline neutrino oscillation experiment. K2K uses an accelerator-produced
muon neutrino beam with a mean energy of 1.3 GeV directed at the
Super-Kamiokande detector.Aliu i Fusté, Ester, American Physical Society, Andringa Dias, Sofia, Aoki, S., Argyriades, J., Asakura, K., Ashie, R., Berns, H., Bhang, H., Blondel, A., Borghi, S., Bouchez, J., Burguet-Castell, J., Casper, D., Cavata, C., Cervera, A., Cho, K.O., Choi, J.H., Dore, U., Espinal Curull, Xavi, Fechner, M., Fernández Sánchez, Enrique, Fukuda, Y., Gomez-Cadenas, J., Gran, R., Hara, T., Hasegawa, M., Hasegawa, T., Hayashi, K., Hayato, Y., Helmer, R.L., Hill, J., Hiraide, K., Hosaka, J., Ichikawa, A.K., Iinuma, M., Ikeda, A., Inagaki, T., Ishida, T., Ishihara, K., Ishii, T., Ishitsuka, M., Itow, Y., Iwashita, T., Jang, H.I., Jeon, E.J., Jeong, I.S., Joo, K., Jover Mañas, Gabriel Vicent, Jung, C.K., K2K Collaboration, Kajita, T., Kameda, J., Kaneyuki, K., Kato, I., Kearns, E., Kerr, D., Khabibullin, M., Khotjantsev, A., Kielczewska, D., Kim, C.O., Kim, J.Y., Kim, S., Kitching, P., Kobayashi, K., Kobayashi, T., Konaka, A., Koshio, Y., Kropp, W., Kubota, J., Kudenko, Yu., Kuno, Y., Kutter, T., Learned, J., Likhoded, S., Lim, I.T., Loverre, P.F., Ludovici, L., Maesaka, H., Mallet, J., Mariani, C., Maruyama, T., Matsuno, S., Matveev, V., Mauger, C., McConnel Mahn, Kendall Brianna, McGrew, C., Mikheyev, S., Minamino, A., Mine, S., Mineev, O., Mitsuda, C., Miura, M., Moriguchi, Y., Morita, T., Moriyama, S., Nakadaira, T., Nakahata, M., Nakamura, K., Nakano, I., Nakaya, T., Nakayama, S., Nambu, R., Nambu, T., Nawang, S., Nishikawa, K., Nitta, K., Nova, Federico, Novella, P., Obayashi, Y., Okada, A., Okumura, K., Oser, S.M., Oyama, Y., Pac, M.Y., Pierre, F., Rodríguez Marrero, Ana Yaiza, Saji, C., Sakuda, M., Sarrat, A., Sasaki, T., Scholberg, K., Schroeter, R., Sekiguchi, M., Sharkey, E., Shiozawa, M., Shiraishi, K., Sitjes, G., Smy, M., Sobel, H., Stone, J., Sulak, L., Suzuki, A., Suzuki, Y., Sánchez Nieto, Federico, T'Jampens, S., Takahashi, T., Takenaga, Y., Takeuchi, Y., Taki, K., Takubo, Y., Tamura, N., Tanaka, M., Terri, R., Tornero-Lopez, A., Totsuka, Y., Ueda, S., Vagins, M., Walter, C.W., Wang, W., Wilkes, R.J., Yamada, S., Yamamoto, S., Yanagisawa, C., Yershov, N., Yokoyama, H., Yokoyama, M., Yoo, J., Yoshida, M., Zalipska, J. +159 morecore +4 more sourcesEffects of nonstandard neutrino interactions at PINGU
, 2013 Neutrino oscillation experiments in the past decades have greatly improved
our knowledge on neutrinos by measuring the fundamental neutrino parameters.
The ongoing and upcoming neutrino oscillation experiments are intended to pin
down the neutrino mass ...Ohlsson, Tommy, Zhang, He, Zhou, Shuncore +1 more sourceTowards Complete Neutrino Mixing Matrix and CP-Violation [PDF]
, 2004 The compelling experimental evidences for oscillations of solar, atmospheric
and reactor neutrinos imply the existence of 3-neutrino mixing in vacuum.Abdurashitov, Aguilar-Saavedra, Ahn, Albright, Antusch, Apollonio, Athanassopoulos, Bahcall, Bandyopadhyay, Bandyopadhyay, Bandyopadhyay, Bandyopadhyay, Barger, Beacom, Bernabeu, Bilenky, Bilenky, Bilenky, Bilenky, Bilenky, Bilenky, Boehm, Burguet-Castell, Choubey, Cleveland, Czakon, Doi, Eguchi, Frampton, Frampton, Fukuda, Gribov, Huber, Jarlskog, Kayser, Krastev, Krastev, Langacker, Lisi, Maki, Maltoni, McConnel, Mikhaelyan, Mikheev, Minakata, Minakata, Minakata, Minakata, Miura, Mohapatra, Morales, Nieves, Palomares-Ruiz, Pascoli, Pascoli, Pascoli, Pascoli, Pascoli, Pascoli, Petcov, Petcov, Petcov, Petcov, Petcov, Petcov, Pontecorvo, Pontecorvo, Raidal, Rajasekaran, Rodejohann, S.T. Petcov, Schechter, Sorel, Stech, Vissani, Wolfenstein, Wolfenstein, Yasuda +77 morecore +2 more sources
