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2961por Gapienko, V A, Ammosov, V V, Gapienko, G S, Korotkov, V A, Zaetz, V G, Burkot, W, Coghen, T, Guy, J, Venus, W A, Andryakov, A D, Asratyan, A E, Kaftanov, V S, Kruchinin, S P, Kubantsev, M A, Makhlyoueva, I V, Erriquez, O, Jones, G T, Varvell, K E, Marage, P, Sacton, J, Morrison, Douglas Robert Ogston, Neveu, M, Wittek, WEnlace del recurso
Publicado 1992
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2962
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2963
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2964por McNulty, R“…A review of measurements of the tau neutrino mass is presented using results from ALEPH, CLEO, DELPHI and OPAL. …”
Publicado 1999
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2965por Hasert, F J, Aubert, Bernard, Bellotti, E, Bertrand-Coremans, G H, Blum, D, Bonetti, S, Brission, V, Bullock, F W, Cavalli, D, Chounet, L M, Comtet, A, Conta, C, Cundy, Donald C, Degrange, B, Esten, M J, Fiorini, Ettore, Haguenauer, Maurice, Haidt, Dieter, Heusse, P, Jones, T W, Kabe, S, Kluberg, L, Krenz, W, Lagarrigue, A, Lanske, D, Lutz, A M, McKenzie, J, Michette, A G, Morfín, J G, Musset, P, Myatt, Gerald, Nguyen-Khac, U, Orkin-Lecourtois, A, Pascaud, C, Pattison, J B M, Perkins, Donald Hill, Petiau, P, Pomello, N, Pullia, Antonio, Rollier, M, Romano, F, Rousset, A, Sacton, J, Schira, R, Schultze, K, Scott, W G, Sletten, H, Van Doninck, W K, Venus, W A, Vialle, J P, Vilain, P, Von Krogh, J, Wachsmuth, H W, Weerts, HEnlace del recurso
Publicado 1974
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2966por Tadsen, A“…The MUNU experiment has been recently built to measure the neutrino magnetic moment at a reactor. Its central part, at the same time target and detector, is a 1 m/sup 3/ TPC filled with 3 bar of CF/sub 4/. …”
Publicado 1999
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2967
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2968“…Under the assumption that the density variation of the electrons can beapproximated by an exponential function, the solar Mikheyev-Smirnov-Wolfensteineffect is treated for three generations of neutrinos. The generalizedhypergeometric functions that result from the exact solution of this problemare studied in detail, and a method for their numerical evaluation ispresented. …”
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2969
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2970
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2971“…We study the sensitivity of the HELLAZ and Borexino solar neutrino experiments on discriminating the neutrino species nu_e, anti-nu_e, nu_{mu,tau}, anti-nu_{mu,tau}, and nu_{sterile} using the difference in the recoil electron kinetic energy spectra in elastic neutrino-electron scattering. …”
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2972Publicado 2000“…The neutrino, Fermi said, had no mass at all. But the neutrino does interact, slightly, and its importance has grown under the watchful eyes of experimenters and theorists.…”
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2973por Dienes, Keith R.“…After briefly reviewing how such dimensions can lower the fundamental GUT, Planck, and string scales, I then outline how these scenarios lead to a new higher-dimensional seesaw mechanism for generating neutrino oscillations --- perhaps even without neutrino masses. …”
Publicado 2000
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2974“…A detailed description of a Tret'yakov-type magnetic$\beta$--spectrometer with electrostatic acceleration is presented.The instrument is being used for high precision measurements of the$ \beta $--spectra of various isotopes and to search for neutrinomixing and heavy neutrinos with masses up to $100 \,$keV$/c^2$.The relative momentum resolution, obtained with an extendedsource ($ 3 \times 2 \,$cm$^2$) and a large silicon stripdetector, is $ \delta p/p = 6.9 \times 10^{-4} $ (FWHM).The width of the energy band, which can simultaneously be measuredwith this resolution, is typically 50 times larger than thecorresponding width of the energy resolution.The detector delivers pulse-height and one-dimensional positioninformation. …”
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2975“…It has been suggested that ultrahigh energy neutrinos can acquire cross-sections approaching hadronic size if the string scale is as low as 1-10 TeV. …”
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2976
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2977
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2978por Blietschau, J, Morfín, J G, Pohl, M, Welch, J, Bertrand-Coremans, G H, Mulkens, H, Sacton, J, Van Doninck, W K, Matteuzzi, C, Romano, F, Blondel, A, Degrange, B, François, T, Nguyen-Khac, U, van Dam, P, Bonetti, S, Cavalli, D, Pullia, Antonio, Lutz, A M, Pascaud, C, Bullock, F W, Jones, T W, Michette, A GEnlace del recurso
Publicado 1977
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2979
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2980por Autin, Bruno, Cappi, R, Gareyte, Jacques, Garoby, R, Giovannozzi, Massimo, Haseroth, H, Hofmann, I, Martini, M, Métral, Elias, Pirkl, Werner, Prior, C R, Rees, G H, Schönauer, Horst Otto, Senichev, Yu V“…An 8 Hz proton driver for a neutrino factory of 4 MW beam power and an energy of 25-30 GeV is under study at CERN, in parallel with a similar investigation using a 2.2 GeV high-energy linac and an accumulator plus a compressor ring cycling at 75 Hz. …”
Publicado 2000
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