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2521
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2533por Daraktchieva, Z, Lamblin, J, Link, O, Amsler, Claude, Avenier, M, Broggini, C, Busto, J, Cerna, C, Gervasio, G, Jeanneret, J B, Jonkmans, G, Koang, D H, Lebrun, D, Ould-Saada, F, Puglierin, G, Stutz, A, Tadsen, A, Vuilleumier, J L“…Upper limits on the neutrino magnetic moment were derived and are discussed.…”
Publicado 2003
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2534“…The atmospheric neutrino flux calculated with FLUKA was originally limited to 100-200 GeV for statistical reasons. …”
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2535“…We show that the same Planck-scale departures from Lorentz symmetry that lead to a modification of the GZK limit which would be consistent with the observations reported by AGASA, also have significant implications for the evaluation of the Bahcall-Waxman bound on the flux of high-energy neutrinos produced by photo-meson interactions in sources of size not much larger than the proton photo-meson mean free path.…”
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2536“…A future galactic SN can be located several hours before the optical explosion through the MeV-neutrino burst, exploiting the directionality of $nu$-$e$-scattering in a water Cherenkov detector such as Super-Kamiokande. …”
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2537
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2540