中文
相关论文

相关论文: Nonzero $\theta_{13}$ in $SO(3) \rightarrow A_4$ l…

200 篇论文

We present a supersymmetric model of quark and lepton based on $S_4\times Z_3\times Z_4$ flavor symmetry. The $S_4$ symmetry is broken down to Klein four and $Z_3$ subgroups in the neutrino and the charged lepton sectors respectively.…

高能物理 - 唯象学 · 物理学 2009-12-04 Gui-Jun Ding

An attempt is made to explore the possibility for deviations of solar mixing angle ($\theta_{12}$) from tri-bimaximal mixings, without sacrificing the predictions of maximal atmospheric mixing angle ($\theta_{23}=\pi/4$) and zero reactor…

高能物理 - 唯象学 · 物理学 2008-11-26 N. Nimai Singh , Monisa Rajkhowa , Abhijit Borah

We investigate the possibility of expressing the charged leptons and neutrino mass matrices as linear combinations of generators of a single finite group. Constraints imposed on the resulting mixing matrix by current data restrict the group…

高能物理 - 唯象学 · 物理学 2015-06-17 G. K. Leontaris , N. D. Vlachos

The near maximal value for the atmospheric neutrino mixing angle together with the fact that the solar mixing angle satisfies the relation $\sin^2\theta_\odot\simeq {1/3}$ is the basis for the so called tri-bimaximal mixing (tbm) when…

高能物理 - 唯象学 · 物理学 2010-04-06 R. N. Mohapatra , S. Nasri , Hai-Bo Yu

We suggest a simple model, based on the type-I seesaw mechanism, for the lepton mass matrices. The model hinges on an Abelian symmetry which leads to mass matrices with some vanishing matrix elements. The model predicts one massless…

高能物理 - 唯象学 · 物理学 2015-06-04 P. M. Ferreira , L. Lavoura

We show that in theories where neutrino masses arise from type I seesaw formula with three right handed neutrinos and where large atmospheric mixing angle owes its origin to an approximate leptonic $\mu-\tau$ interchange symmetry, the…

高能物理 - 唯象学 · 物理学 2008-11-26 R. N. Mohapatra , S. Nasri , Haibo Yu

The neutrino mixing angle theta(13) is at the focus of current neutrino research. From a global analysis of the available oscillation data in a 3-neutrino framework, we previously reported [Phys. Rev. Lett. 101, 141801 (2008)] hints in…

高能物理 - 唯象学 · 物理学 2013-05-29 G. L. Fogli , E. Lisi , A. Marrone , A. Palazzo , A. M. Rotunno

An alternative supersymmetric SO(10) grand unification model with lopsided fermion mass matrices is introduced. It generates a large solar-neutrino-mixing angle through the neutrinos' Dirac mass matrix constrained by the SO(10) group…

高能物理 - 唯象学 · 物理学 2009-11-11 Xiangdong Ji , Yingchuan Li , R. N. Mohapatra

After the successful determination of the reactor neutrino mixing angle \theta_13 ~ 0.16 \neq 0, a new feature suggested by the current neutrino oscillation data is a sizeable deviation of the atmospheric neutrino mixing angle \theta_23…

高能物理 - 唯象学 · 物理学 2014-01-30 David Marzocca , Serguey T. Petcov , Andrea Romanino , Maria C. Sevilla

Neutrino oscillation data indicate the presence of a 2-3 symmetry for the left-handed neutrinos. We show that this symmetry between the second and third generations cannot be extended to include the charged leptons, no matter what basis we…

高能物理 - 唯象学 · 物理学 2009-11-11 C. S. Lam

We speculate that the mass spectrum of three neutrinos might have a normal hierarchy as that of three charged leptons or that of three up-type (or down-type) quarks. In this spirit, we propose a novel parametrization of the $3\times 3$…

高能物理 - 唯象学 · 物理学 2009-11-11 Harald Fritzsch , Zhi-zhong Xing

We show that a modification of a recently proposed model by Altarelli and Feruglio with softly broken $A_4$ symmetry leads naturally to nonvanishing $U_{e3}$ with $\theta_{13}\simeq 2^o - 4^o$. The observed mass squared differences for…

高能物理 - 唯象学 · 物理学 2011-05-05 Biswajit Adhikary , Biswajoy Brahmachari , Ambar Ghosal , Ernest Ma , M. K. Parida

We present a model for leptonic mixing and the lepton masses based on flavor symmetries and higher-dimensional mass operators. The model predicts bilarge leptonic mixing (i.e., the mixing angles theta_{12} and theta_{23} are large and the…

高能物理 - 唯象学 · 物理学 2009-11-07 Tommy Ohlsson , Gerhart Seidl

The neutrino mixing matrix U is in general of the form U=U_e^+ U_nu, where U_e arises from the diagonalization of charged leptons and U_nu is from the neutrino sector. We discuss the possibility that U_nu is nearly diagonal (in the…

高能物理 - 唯象学 · 物理学 2010-04-05 Guido Altarelli , Ferruccio Feruglio , Isabella Masina

We propose a new scenario in a radiative seesaw model based on A_4 flavor symmetry. In this model, we explore a possibility of linking non-zero \theta_{13} to dark matter. And we analyze the lepton sector to predict the observed neutrinos…

高能物理 - 唯象学 · 物理学 2015-06-03 Y. H. Ahn , Hiroshi Okada

Many experiments are being planned to measure the neutrino mixing parameter $\theta_{13}$ using reactor as well as accelerator neutrino beams. In this note, the theoretical significance of a high precision measurement of this parameter is…

高能物理 - 唯象学 · 物理学 2008-11-26 R. N. Mohapatra

It has been shown that the Cabibbo angle can be predicted in terms of group theoretical quantities, if the dihedral group D14 plays the role of a flavor symmetry. We extend a supersymmetric D14 model to the lepton sector and show that…

高能物理 - 唯象学 · 物理学 2015-06-04 C. Hagedorn , D. Meloni

Recent work on a lepton mass matrix model based on an SU(3) flavor symmetry which is broken into S_4 is reviewed. The flavor structures of the masses and mixing are caused by VEVs of SU(2)_L-singlet scalars \phi which are nonets ({\bf…

高能物理 - 唯象学 · 物理学 2007-07-09 Yoshio Koide

We study perturbations of exactly tri-bimaximal neutrino mixings under the assumption that they are coming solely from the charged lepton mass matrix. This may be plausible in scenarios where the mass generation mechanisms of neutrinos and…

高能物理 - 唯象学 · 物理学 2015-05-20 Davide Meloni , Florian Plentinger , Walter Winter

We update the analysis of the viability of the lepton mixing patterns originating from $A_4$, $S_4$ and $A_5$ discrete flavour symmetries and leading to predictions for the solar neutrino mixing angle, $\theta_{12}$. We perform a…

高能物理 - 唯象学 · 物理学 2026-03-19 S. T. Petcov , A. V. Titov