Results 41 to 50 of about 1,071,967 (270)
Search for sterile neutrino mixing using three years of IceCube DeepCore data [PDF]
, 2017 We present a search for a light sterile neutrino using three years of atmospheric neutrino data from the DeepCore detector in the energy range of approximately 10-60 GeV.I. C. M. Aartsen, M. Ackermann, J. Adams, J. Aguilar, M. Ahlers, M. Ahrens, I. A. Samarai, D. Altmann, K. Andeen, T. Anderson, I. Ansseau, G. Anton, M. Archinger, C. Arguelles, J. Auffenberg, S. Axani, X. Bai, S. Barwick, V. Baum, R. Bay, J. Beatty, J. Tjus, K. Becker, S. Benzvi, D. Berley, E. Bernardini, D. Besson, G. Binder, D. Bindig, E. Blaufuss, S. Blot, C. Bohm, M. Borner, F. Bos, D. Bose, S. Boser, O. Botner, J. Braun, L. Brayeur, H. Bretz, S. Bron, A. Burgman, T. Carver, M. Casier, E. Cheung, D. Chirkin, A. Christov, K. Clark, L. Classen, S. Coenders, G. Collin, J. Conrad, D. Cowen, R. Cross, M. Day, J. Andr'e, C. Clercq, E. del Pino Rosendo, H. Dembinski, S. Ridder, P. Desiati, K. D. Vries, G. Wasseige, M. With, T. DeYoung, J. C. D'iaz-V'elez, V. Lorenzo, H. Dujmovic, J. Dumm, M. Dunkman, B. Eberhardt, T. Ehrhardt, B. Eichmann, P. Eller, S. Euler, P. Evenson, S. Fahey, A. Fazely, J. Feintzeig, J. Felde, K. Filimonov, C. Finley, S. Flis, C.-C. Fosig, A. Franckowiak, E. Friedman, T. Fuchs, T. Gaisser, J. Gallagher, L. Gerhardt, K. Ghorbani, W. Giang, L. Gladstone, T. Glauch, T. Glusenkamp, A. Goldschmidt, J. G. Gonzalez, D. Grant, Z. Griffith, C. Haack, A. Hallgren, F. Halzen, E. Hansen, T. Hansmann, K. Hanson, D. Hebecker, D. Heereman, K. Helbing, R. Hellauer, S. Hickford, J. Hignight, G. Hill, K. Hoffman, R. Hoffmann, K. Hoshina, F. Huang, M. Huber, K. Hultqvist, S. In, A. Ishihara, E. Jacobi, G. Japaridze, M. Jeong, K. Jero, B. Jones, W. Kang, A. Kappes, T. Karg, A. Karle, U. Katz, M. Kauer, A. Keivani, J. Kelley, A. Kheirandish, J. Kim, M. Kim, T. Kintscher, J. Kiryluk, T. Kittler, S. Klein, G. Kohnen, R. Koirala, H. Kolanoski, R. Konietz, L. Kopke, C. Kopper, S. Kopper, D. Koskinen, M. Kowalski, K. Krings, M. Kroll, G. Kruckl, C. Kruger, J. Kunnen, S. Kunwar, N. Kurahashi, T. Kuwabara, A. Kyriacou, M. Labare, J. Lanfranchi, M. Larson, F. Lauber, D. Lennarz, M. Lesiak-Bzdak, M. Leuermann, L. Lu, J. Lunemann, J. Madsen, G. Maggi, K. Mahn, S. Mancina, M. Mandelartz, R. Maruyama, K. Mase, R. Maunu, F. McNally, K. Meagher, M. Medici, M. Meier, T. Menne, G. Merino, T. Meures, S. Miarecki, J. Micallef, G. Moment'e, T. Montaruli, M. Moulai, R. Nahnhauer, U. Naumann, G. Neer, H. Niederhausen, S. Nowicki, D. Nygren, A. Pollmann, A. Olivas, A. O'Murchadha, T. Palczewski, H. Pandya, D. Pankova, P. Peiffer, O. Penek, J. Pepper, C. Heros, D. Pieloth, E. Pinat, P. Price, G. Przybylski, M. Quinnan, C. Raab, L. Radel, M. Rameez, K. Rawlins, R. Reimann, B. Relethford, M. Relich, E. Resconi, W. Rhode, M. Richman, B. Riedel, S. Robertson, M. Rongen, C. Rott, T. Ruhe, D. Ryckbosch, D. Rysewyk, L. Sabbatini, S. Herrera, A. Sandrock, J. Sandroos, S. Sarkar, K. Satalecka, P. Schlunder, T. Schmidt, S. Schoenen, S. Schoneberg, L. Schumacher, D. Seckel, S. Seunarine, D. Soldin, M. Song, G. Spiczak, C. Spiering, J. Stachurska, T. Stanev, Alexander Stasik, J. Stettner, A. Steuer, T. Stezelberger, R. Stokstad, A. Stossl, R. Strom, N. Strotjohann, G. Sullivan, M. Sutherland, H. Taavola, I. Taboada, J. Tatar, F. Tenholt, S. Ter-Antonyan, A. Terliuk, G. Tevsi'c, S. Tilav, P. Toale, M. Tobin, S. Toscano, D. Tosi, M. Tselengidou, C. Tung, A. Turcati, E. Unger, M. Usner, J. Vandenbroucke, N. Eijndhoven, S. Vanheule, M. Rossem, J. Santen, M. Vehring, M. Voge, E. Vogel, M. Vraeghe, C. Walck, A. Wallace, M. Wallraff, N. Wandkowsky, A. Waza, C. Weaver, M. Weiss, C. Wendt, S. Westerhoff, B. Whelan, S. Wickmann, K. Wiebe, C. Wiebusch, L. Wille, D. Williams, L. Wills, M. Wolf, T. R. Wood, E. Woolsey, K. Woschnagg, D. Xu, X. Xu, Y. Xu, J. Yáñez, G. Yodh, S. Yoshida, M. Zoll +306 moresemanticscholar +1 more sourceNeutrino 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 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 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 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 sourceNeutrino mixing and cosmology [PDF]
Nuclear Physics B - Proceedings Supplements, 2005 We review the consequences of neutrino mixing in the early universe. For both active-sterile mixing or mixing between three active neutrinos only, the consequences of oscillations depend crucially upon the size of the universe's lepton number (relic neutrino asymmetry.)openaire +3 more sources
