Predictive model of radiative neutrino masses

被引:15
|
作者
Babu, K. S. [1 ]
Julio, J. [2 ]
机构
[1] Oklahoma State Univ, Dept Phys, Stillwater, OK 74078 USA
[2] Jozef Stefan Inst, Ljubljana 1001, Slovenia
来源
PHYSICAL REVIEW D | 2014年 / 89卷 / 05期
关键词
ZEE MODEL; MATRIX;
D O I
10.1103/PhysRevD.89.053004
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a simple and predictive model of radiative neutrino masses. It is a special case of the Zee model which introduces two Higgs doublets and a charged singlet. We impose a family-dependent Z(4) symmetry acting on the leptons, which reduces the number of parameters describing neutrino oscillations to four. A variety of predictions follow: the hierarchy of neutrino masses must be inverted; the lightest neutrino mass is extremely small and calculable; one of the neutrino mixing angles is determined in terms of the other two; the phase parameters take CP-conserving values with delta(CP) = pi; and the effective mass in neutrinoless double beta decay lies in a narrow range, m(beta beta) = (17.6-18.5) meV. The ratio of vacuum expectation values of the two Higgs doublets, tan beta, is determined to be either 1.9 or 0.19 from neutrino oscillation data. Flavor-conserving and flavor-changing couplings of the Higgs doublets are also determined from neutrino data. The nonstandard neutral Higgs bosons, if they are moderately heavy, would decay dominantly into and t with prescribed branching ratios. Observable rates for the decays. mu -> e gamma and iota -> 3 mu are predicted if these scalars have masses in the range of 150-500 GeV.
引用
收藏
页数:11
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