Flavor Symmetries, Neutrino Masses and Neutrino Mixing

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dc.creatorFritzsch, H.
dc.date2008-02-07
dc.date.accessioned2026-07-07T11:55:54Z
dc.date.available2026-07-07T11:55:54Z
dc.descriptionWe discuss the neutrino mixing, using the texture 0 mass matrices, which work very well for the quarks. The solar mixing angle is directly linked to the mass ratio of the first two neutrinos. The neutrino masses are hierarchical, but the mass ratios turn out to be much smaller than for quarks. The atmospheric mixing angle is 38$^{\circ}$. The CP violation for leptons should be much smaller than for quarks.
dc.description4 pages
dc.identifierhttps://arxiv.org/abs/0802.0937
dc.identifierhttp://arxiv.org/abs/0802.0937
dc.identifierInt.J.Mod.Phys.A23:3179-3182,2008
dc.identifierdoi:10.1142/S0217751X08041773
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/205400
dc.subjectHigh Energy Physics - Phenomenology
dc.titleFlavor Symmetries, Neutrino Masses and Neutrino Mixing
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