机构地区:[1]School of Physics,Shandong University [2]Institute of High Energy Physics,Chinese Academy of Sciences [3]School of Physical Sciences,University of Chinese Academy of Sciences [4]Center for High Energy Physics,Peking University
出 处:《Chinese Physics C》2017年第11期44-55,共12页中国物理C(英文版)
基 金:Supported by NNSFC(11325525);National Recruitment Program for Young Professionals;CAS Center for Excellence in Particle Physics(CCEPP)
摘 要:In the framework of the canonical seesaw model,we present a simple but viable scenario to explicitly break an S3L×S3R flavor symmetry in the leptonic sector.It turns out that the leptonic flavor mixing matrix is completely determined by the mass ratios of the charged leptons(i.e.,me/mμand mμ/mτ) and those of light neutrinos(i.e.,m1/m2 and m2/m3).The latest global-fit results of the three neutrino mixing angles {θ12,θ13,θ23}and two neutrino mass-squared differences {?m212,?m312} at the 3σ level are used to constrain the parameter space of {m1/m2,m2/m3}.The predictions for the mass spectrum and flavor mixing are highlighted:(1) the neutrino mass spectrum shows a hierarchical pattern and a normal ordering,e.g.,m1≈2.2meV,m2≈8.8 meV and m3≈52.7 meV;(2) only the first octant of θ23 is allowed,namely,41.8? θ23 43.3?;(3) the Dirac C P-violating phase δ ≈-22?deviates significantly from the maximal value-90?.All these predictions are ready to be tested in ongoing and forthcoming neutrino oscillation experiments.Moreover,we demonstrate that the cosmological matter-antimatter asymmetry can be explained via resonant leptogenesis,including the individual lepton-flavor effects.In our scenario,leptonic C P violation at low-and high-energy scales is closely connected.In the framework of the canonical seesaw model,we present a simple but viable scenario to explicitly break an S3L×S3R flavor symmetry in the leptonic sector.It turns out that the leptonic flavor mixing matrix is completely determined by the mass ratios of the charged leptons(i.e.,me/mμand mμ/mτ) and those of light neutrinos(i.e.,m1/m2 and m2/m3).The latest global-fit results of the three neutrino mixing angles {θ12,θ13,θ23}and two neutrino mass-squared differences {?m212,?m312} at the 3σ level are used to constrain the parameter space of {m1/m2,m2/m3}.The predictions for the mass spectrum and flavor mixing are highlighted:(1) the neutrino mass spectrum shows a hierarchical pattern and a normal ordering,e.g.,m1≈2.2meV,m2≈8.8 meV and m3≈52.7 meV;(2) only the first octant of θ23 is allowed,namely,41.8? θ23 43.3?;(3) the Dirac C P-violating phase δ ≈-22?deviates significantly from the maximal value-90?.All these predictions are ready to be tested in ongoing and forthcoming neutrino oscillation experiments.Moreover,we demonstrate that the cosmological matter-antimatter asymmetry can be explained via resonant leptogenesis,including the individual lepton-flavor effects.In our scenario,leptonic C P violation at low-and high-energy scales is closely connected.
关 键 词:canonical seesaw model S3L× S3R flavor symmetry leptonic CP violation cosmological matter-antimatter asymmetry resonant leptogenesis
分 类 号:O572.321[理学—粒子物理与原子核物理]
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