Results 41 to 50 of about 1,121,622 (286)
Maximal Neutrino Mixing from an Attractive Infrared Fixed Point [PDF]
, 2001 In the Standard Model (and MSSM), renormalization effects on neutrino mixing
are generally very small and the attractive fixed points are at vanishing
neutrino mixing.Abdurashitov, Ahmad, Apollonio, Babu, Balaji, Borzumati, Casas, Casas, Chankowski, Chankowski, Cleveland, Ellis, Flores, Fogli, Fukuda, Fukuda, Ghosal, Glashow, Guo-Hong Wu, Haba, Haba, Haba, Hampel, Hatakeyama, Hill, James Pantaleone, Jarlskog, Kanemura, Kanemura, King, Koide, Komatsu, Kominis, Kuo, Kuo, Kuo, Lebedev, Nie, Pantaleone, Peccei, Schrempp, Sher, Strogatz, T.K Kuo, Tanimoto, Weinberg, Xing, Zee, Zee +48 morecore +3 more sourcesNeutrino masses and neutrino mixing
Nuclear Physics B - Proceedings Supplements, 2006 We review the current (summer 2005) status of neutrino mass and mixing parameters, as emerging from a phenomenological analysis of world neutrino oscillation and non-oscillation data, performed within the standard three-neutrino mixing framework.Antonio Marrone, Antonio Palazzo, G. L. Fogli, Eligio Lisi, A. M. Rotunno +4 moreopenaire +3 more sourcesSearch for active-sterile neutrino mixing using neutral-current interactions in NOvA [PDF]
, 2017 We report results from the first search for sterile neutrinos mixing with active neutrinos through a reduction in the rate of neutral-current interactions over a baseline of 810 km between the NOvA detectors.NOvA Collaboration P. Adamson, L. Aliaga, D. Ambrose, N. Anfimov, A. Antoshkin, E. Arrieta-Diaz, K. Augsten, A. Aurisano, C. Backhouse, M. Baird, B. Bambah, K. Bays, B. Behera, S. Bending, R. Bernstein, V. Bhatnagar, B. Bhuyan, J. Bian, T. Blackburn, A. Bolshakova, C. Bromberg, J. Brown, G. Brunetti, N. Buchanan, A. Butkevich, V. Bychkov, M. Campbell, E. Catano-Mur, S. Childress, B. Choudhary, B. Chowdhury, T. Coan, J. Coelho, M. Colo, J. Cooper, L. Corwin, L. Cremonesi, D. Cronin-Hennessy, G. Davies, J. Davies, P. Derwent, R. Dharmapalan, P. Ding, Z. Djurcic, E. Dukes, H. Duyang, S. Edayath, R. Ehrlich, G. Feldman, M. Frank, M. Gabrielyan, H. Gallagher, S. Germani, T. Ghosh, A. Giri, R. Gomes, M. Goodman, V. Grichine, M. Groh, R. Group, D. Grover, B. Guo, A. Habig, J. Hartnell, R. Hatcher, A. Hatzikoutelis, K. Heller, A. Himmel, A. Holin, B. Howard, J. Hylen, F. Jediný, M. Judah, G. Kafka, D. Kalra, S. Amcix, S. Kasetti, R. Keloth, L. Kolupaeva, S. Kotelnikov, I. Kourbanis, A. Kreymer, A. Kumar, S. Kurbanov, T. Lackey, K. Lang, W. Lee, S. Lin, M. Lokajicek, J. Lozier, S. Luchuk, K. Maan, S. Magill, W. Mann, M. Marshak, K. Matera, V. Matveev, D. M'endez, M. Messier, H. Meyer, T. Miao, W. Miller, S. Mishra, R. Mohanta, A. Moren, L. Mualem, M. Muether, S. Mufson, R. Murphy, J. Musser, J. Nelson, R. Nichol, E. Niner, A. Norman, T. Nosek, Y. Oksuzian, A. Olshevskiy, T. Olson, J. Paley, R. Patterson, G. Pawloski, D. Pershey, O. Petrova, R. Petti, S. Phan-Budd, R. Plunkett, R. Poling, B. Potukuchi, C. Principato, F. Psihas, A. Radovic, R. Rameika, B. Rebel, B. Reed, D. Rocco, P. Rojas, V. Ryabov, K. Sachdev, P. Sail, O. Samoylov, M. Sánchez, R. Schroeter, J. Sepulveda-Quiroz, P. Shanahan, A. Sheshukov, J. Singh, P. Singh, V. Singh, J. Smolík, N. Solomey, E. Song, A. Sousa, K. Soustruznik, M. Strait, L. Suter, R. Talaga, P. Tas, R. B. Thayyullathil, J. Thomas, X. Tian, S. Tognini, J. Tripathi, A. Tsaris, J. Urheim, P. Vahle, J. Vasel, L. Vinton, A. Vold, T. Vrba, B. Wang, M. Wetstein, D. Whittington, S. Wojcicki, J. Wolcott, N. Yadav, S. Yang, J. Zálešák, B. Zamorano, R. Zwaska +178 moresemanticscholar +1 more sourceSearch for heavy neutrinos mixing with tau neutrinos [PDF]
Physics Letters B, 2001 We report on a search for heavy neutrinos ($\nus$) produced in the decay $D_s\to \nus$ at the SPS proton target followed by the decay $\nudecay$ in the NOMAD detector. Both decays are expected to occur if $\nus$ is a component of $ _ $.\ From the analysis of the data collected during the 1996-1998 runs with $4.1\times10^{19}$ protons on target, a ...Giacomo Graziani, Marco Fraternali, L. S. Peak, A. Kovzelev, Caren Hagner, J.-P. Mendiburu, Barry Blumenfeld, Marco Laveder, L. Vacavant, G. Vidal-Sitjes, G. Vidal-Sitjes, L. La Rotonda, I. Bird, I. Bird, M. Baldo-Ceolin, D. Gibin, M. Mezzetto, J. Rico, T. Fazio, P. Zuccon, J.-M. Levy, N.V. Krasnikov, H. Degaudenzi, F. J. P. Soler, F. J. P. Soler, J. M. Gaillard, A. Marchionni, J.J. Gómez-Cadenas, J.J. Gómez-Cadenas, A. Letessier-Selvon, B. Lakić, Bruce Yabsley, G. N. Taylor, C. Lachaud, G. J. Feldman, J.-M. Vieira, Th. Stolarczyk, L. Linssen, Alessandro Cardini, G. Bassompierre, C. Conta, O. Klimov, A. Guglielmi, K. Schahmaneche, M. Banner, A. Grant, E. Iacopini, Valerio Vercesi, A. Krasnoperov, A. Krasnoperov, Malcolm Ellis, J. Ulrichs, J. Long, E. Gangler, E. Gangler, D. Steele, D. Steele, P. Rathouit, M. Kirsanov, S. Boyd, N. Hyett, J. Bouchez, F. Vannucci, B. Schmidt, B. Schmidt, J. Gosset, Yu. Nefedov, Kevin Varvell, A. Cervera-Villanueva, A. Cervera-Villanueva, P. Hurst, M. T. Tran, Claus Gößling, Stefano Lacaprara, L. Camilleri, Dmitry V. Naumov, Vincenzo Cavasinni, D. Pollmann, V. Flaminio, A. Baldisseri, Domizia Orestano, J. Dumarchez, A. De Santo, A.-M. Touchard, E. do Couto e Silva, A. Polyarush, M. C. Gonzalez-Garcia, M. Contalbrigo, H. Zaccone, S.R. Mishra, S.R. Mishra, L.J. Winton, T. Del Prete, M. Tareb-Reyes, Caroline Poulsen, F. Martelli, S.A. Bunyatov, Giacomo Polesello, A. Lanza, F. Salvatore, André Rubbia, André Rubbia, A. Godley, D. Hubbard, J. A. Hernando, P.W. Cattaneo, C. Nguyen-Mau, P. Nédélec, F. Bobisut, R. Cousins, Mario Stipčević, Nathalie Besson, S. N. Tovey, Antonio Bueno, Antonio Bueno, P. Astier, D. Daniels, H. Pessard, M. Veltri, A. N. Toropin, R. Petti, J. Kokkonen, V. Tereshchenko, C. Joseph, K. Benslama, Fr Pastore, M. Valdata-Nappi, M. Valdata-Nappi, Ante Ljubičić, A. Placci, F. Juget, G. Collazuol, L. Di Lella, G. Sozzi, Kai Zuber, Achim Geiser, Achim Geiser, Sergei Gninenko, Sergei Gninenko, Chiara Roda, Chiara Roda, D. Autiero, Didier Ferrere, I.J. Donnelly, G. F. Moorhead, Fergus Wilson, E. Tsesmelis, G. Conforto, U. Stiegler, G. Segneri, A. Lupi, M. E. Sevior, E. Pennacchio, X. Méchain, T. Vinogradova, Roberto Ferrari, Vyacheslav Valuev, Vyacheslav Valuev, M. Gouanère, T. Dignan, T. Weisse, J-P. Meyer, B. A. Popov, B. A. Popov, D. Geppert, F.V. Weber, F.V. Weber +166 moreopenaire +6 more sourcesA Phenomenological Study on Lepton Mass Matrix Textures [PDF]
, 2001 The three active light neutrinos are used to explain the neutrino
oscillations. The inherently bi-large mixing neutrino mass matrix and the
Fritzsch type, bi-small mixing charged lepton mass matrix are assumed.A. Aranda, A. Baltz, A. Strumia, C. Giunti, C. H. Albright, C. Jarlskog, C. Jarlskog, C. S. Kim, Chun Liu, D. E. Groom, D. Falcone, D. V. Ahluwalia, D.-D. Wu, E. Torrente-Lujan, H. B. Benaoum, H. Fritzsch, H. Fritzsch, H. Fritzsch, H. Fritzsch, H. Georgi, Jeonghyeon Song, K. Choi, M. Buchmuller, M. C. Gonzales-Garcia, M. Fukugita, M. Jezabek, M. Lindner, M.-C. Chen, P. Greminelli, Q. R. Ahmad, R. Barbieri, R. N. Mohapatra, R. N. Mohapatra, S. Davidson, S. Davidson, S. K. Kang, S. M. Barr, V. Barger, Y. Fukuda, Y. Fukuda, Y. Koide, Y.-L. Wu, Z.-Z. Xing +42 morecore +3 more sourcesMajorana neutrino mixing [PDF]
Journal of Physics G: Nuclear and Particle Physics, 2006 The most plausible see-saw explanation of the smallness of the neutrino masses is based on the assumption that total lepton number is violated at a large scale and neutrinos with definite masses are Majorana particles. In this review we consider in details difference between Dirac and Majorana neutrino mixing and possibilities of revealing Majorana ...openaire +3 more sources