Bi-Large Neutrino Mixing See-Saw Mass Matrix with Texture Zeros and Leptogenesis

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dc.creatorChao, Wei
dc.creatorHe, Xiao-Gang
dc.creatorLi, Xue-Qian
dc.date2005-03-30
dc.date2005-06-05
dc.date.accessioned2026-07-07T11:58:34Z
dc.date.available2026-07-07T11:58:34Z
dc.descriptionWe study constraints on neutrino properties from texture zeros in bi-large mixing See-Saw mass matrix and also from leptogenesis. Texture zeros may occur in the light (class a)) or in the heavy (class b)) neutrino mass matrices. Each of these two classes has 5 different forms which can produce non-trivial three generation mixing with at least one texture zero. We find that two types of texture zero mass matrices in both class a) and class b) can be consistent with present data on neutrino masses, mixing and produce the observed baryon asymmetry of the universe. None of the neutrinos can have zero masses with the lightest of the light neutrinos having a mass larger than about 0.039 eV for class a) and 0.002 eV for class b). In these models although CKM CP violating phase vanishes, non-zero Majorana phases, however, can exist and play an important role in producing the observed baryon asymmetry in our universe through leptogenesis mechanism. The requirement of producing the observed baryon asymmetry can further distinguish different models and also restrict the See-Saw scale to be in the range $10^{12}\sim 10^{15}$ GeV.
dc.description21 pages, 7 figures revised version, some references added, to be submitted to PRD
dc.identifierhttps://arxiv.org/abs/hep-ph/0503285
dc.identifierhttp://arxiv.org/abs/hep-ph/0503285
dc.identifierCommun.Theor.Phys.45:1073-1084,2006
dc.identifierdoi:10.1088/0253-6102/45/6/023
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/206271
dc.subjectHigh Energy Physics - Phenomenology
dc.titleBi-Large Neutrino Mixing See-Saw Mass Matrix with Texture Zeros and Leptogenesis
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