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3141
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3142“…In view of the recent results from the MiniBooNE experiment we revisit the global neutrino oscillation fit to short-baseline neutrino data by adding one or two sterile neutrinos with eV-scale masses to the three Standard Model neutrinos, and for the first time we consider also the global fit with three sterile neutrinos. …”
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3143“…The beta beam concept for the production of intense (anti-)neutrino beams is now well established. A baseline design has recently been published for a beta-beam facility at CERN. …”
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3144
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3145por Uiterwijk, J W E“…The chorus experiment has been used to study neutrino oscillations using the neutrino beam at cern. …”
Publicado 2007
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3146
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3147por Hajdukovic, Dragan Slavkov“…First, the supermassive black hole in the center of our Galaxy (Southern Sky)and in the center of the Andromeda Galaxy (Northern Sky)may produce a flux of antineutrinos measurable with the new generation of the neutrino telescopes; like the IceCube Neutrino Detector under construction at the South Pole, and the future one cubic kilometer telescope in Mediterranean Sea. …”
Publicado 2007
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3148“…We study nuclear effects in charged current deep inelastic neutrino--iron scattering in the framework of a chi^2-analysis of parton distribution functions. …”
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3149
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3150
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3151
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3152“…Here, we concentrate on massive (mostly sterile) neutrinos heavier than 1 MeV.…”
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3153por Kayis-Topaksu, A., Onengut, G., van Dantzig, Rene, de Jong, M., Oldeman, R.G.C., Guler, M., Kama, S., Kose, U., Serin-Zeyrek, M., Tolun, P., Catanesi, M.G., Muciaccia, M.T., Bulte, A., Winter, K., Van de Vyver, B., Vilain, P., Wilquet, G., Saitta, B., Di Capua, E., Ogawa, S., Shibuya, H., Hristova, I.R., Kawamura, T., Kolev, D., Litmaath, M., Meinhard, H., Panman, J., Rozanov, Alexandre N., Tsenov, Roumen Vassilev, Uiterwijk, J.W.E., Zucchelli, P., Goldberg, J., Chikawa, M., Song, J.S., Yoon, C.S., Kodama, K., Ushida, N., Aoki, S., Hara, T., Delbar, T., Favart, Denis, Gregoire, Ghislain Simon, Kalinin, S., Makhlioueva, I., Artamonov, A., Gorbunov, P., Khovansky, V., Shamanov, V., Tsukerman, I., Bruski, N., Frekers, D., Rondeshagen, D., Wolff, T., Hoshino, Kaoru, Kawada, J., Komatsu, M., Miyanishi, M., Nakamura, M., Nakano, T., Narita, K., Niu, K., Niwa, K., Nonaka, N., Sato, O., Toshito, T., Buontempo, S., Cocco, Alfredo G., D'Ambrosio, N., De Lellis, G., De Rosa, G., Di Capua, F., Fiorillo, Giuliana, Marotta, A., Messina, M., Migliozzi, P., Santorelli, R., Scotto Lavina, L., Strolin, Paolo Emilio, Tioukov, V., Okusawa, Toru, Dore, U., Loverre, P.F., Ludovici, Lucio, Rosa, G., Santacesaria, Roberta, Satta, A., Spada, F.R., Barbuto, E., Bozza, C., Grella, G., Romano, G., Sirignano, C., Sorrentino, S., Sato, Y., Tezuka, I.“…The results are based on a sample of 8910 neutrino and 430 antineutrino induced opposite-sign dimuon events collected during the exposure of the detector to the CERN Wide Band Neutrino Beam between 1995 and 1998. …”
Publicado 2008
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3154“…Lepton-flavour symmetry in the Standard Model is broken by small masses for charged leptons and neutrinos. Introducing neutrino masses via dimension-5 operators associated to lepton-number violation at a very high scale, the corresponding coupling matrix may still have entries of order 1, resembling the situation in the quark sector with large top Yukawa coupling. …”
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3155“…We study the potential of future high energy e+e- colliders to probe excited neutrino signals in different channels coming from the single production process via gauge interactions. …”
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3156por McElrath, Bob“…We point out that the Pauli blocking of neutrinos by cosmological relic neutrinos can be a significant effect. …”
Publicado 2009
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3157
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3158por Nakamoto, T“…Superconducting combined function magnets will be utilized for the 50 GeV, 750 kW proton beam line for the J-PARC neutrino experiment. The magnet is designed to provide a dipole field of 2.6 T combined with a quadrupole field of 19 T/m in a coil aperture of 173.4 mm at a nominal current of 7345 A. …”
Publicado 2009
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3159“…The only fine tuning needed in the model is to reproduce the small observed value of r, the ratio between the neutrino mass squared differences. Once the relevant parameters are set to accommodate r then the spectrum of light neutrinos shows a moderate normal hierarchy and is compatible, within large ambiguities, with the constraints from leptogenesis as an explanation of the baryon asymmetry in the Universe.…”
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3160“…As a consequence the predicted value of $\theta_{13}$ is within the sensitivity of the experiments which will take data in the near future. The light neutrino spectrum, typical of $A_4$ see-saw models, with its phenomenological implications, also including leptoproduction, is studied in detail.…”
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