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相关论文: Neutrino masses and mixing in $A_5$ with flavour a…

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Best-fit values of recent global analyzes of neutrino data imply large solar neutrino mixing, vanishing U_{e3} and a non-maximal atmospheric neutrino mixing angle theta_{23}. We show that these values emerge naturally by the hypothesis of…

高能物理 - 唯象学 · 物理学 2008-11-26 A. Blum , R. N. Mohapatra , W. Rodejohann

On account of the new neutrino oscillation data signalling a non-zero value for the smallest mixing angle ($\theta_z$), we present an explicit realization of the underlying U(1) symmetry characterizing the maximal atmospheric mixing angle…

高能物理 - 唯象学 · 物理学 2013-05-30 E. I. Lashin , N. Chamoun , S. Nasri

A non-supersymmetric inverse seesaw model of neutrino mass based on the $A^{\prime}_5$ modular symmetry is presented. This framework provides a combined explanation for neutrino masses, mixing, and the cosmic baryon asymmetry through…

高能物理 - 唯象学 · 物理学 2026-03-20 Xianshuo Zhang , Yakefu Reyimuaji

We analyze the structure of quark and lepton mass matrices under the hypothesis that they are determined from a minimum principle applied to a generic potential invariant under the $\left[SU(3)\right]^5\otimes \mathcal O(3)$ flavor…

高能物理 - 唯象学 · 物理学 2015-06-16 R. Alonso , M. B. Gavela , G. Isidori , L. Maiani

We study the effects of breaking S3 symmetry in the neutrino mass matrix for the masses and mixing matrix of neutrinos. At zeroth order the model gives degenerate neutrino masses and accommodates tribimaximal mixing. We introduce…

高能物理 - 唯象学 · 物理学 2012-02-16 S. Dev , Radha Raman Gautam , Lal Singh

The discrete non-Abelian symmetry $A_4$, valid at some high-energy scale, naturally leads to degenerate neutrino masses, without spoiling the hierarchy of charged-lepton masses. Realistic neutrino mass splittings and mixing angles (one of…

高能物理 - 唯象学 · 物理学 2009-09-17 K. S. Babu , Ernest Ma , J. W. F. Valle

We consider the problem of neutrino masses and mixing angles in a supersymmetric model based on the gauge group SU(4)$\otimes$SU(2)$_L\otimes$SU(2)$_R$ broken at the scale $M_X\approx 10^{16}$ GeV. We extend a previous operator analysis of…

高能物理 - 唯象学 · 物理学 2009-10-28 B. C. Allanach , S. F. King

We present a model for lepton masses and mixing angles using the deconstruction setup, based on a non-Abelian flavor symmetry which is a split extension of the Klein group. The symmetries enforce an approximately maximal atmospheric mixing…

高能物理 - 唯象学 · 物理学 2007-05-23 Gerhart Seidl

If the generating mechanism for neutrino mass is to account for both the newly observed muon anomalous magnetic moment as well as the present experimental bounds on lepton flavor nonconservation, then the neutrino mass matrix should be…

高能物理 - 唯象学 · 物理学 2009-11-07 Ernest Ma , Martti Raidal

The mass matrices of the charged leptons and neutrinos, that had been derived in the framework of a Minimal S_3-invariant Extension of the Standard Model, are here reparametrized in terms of their eigenvalues. The neutrino mixing matrix,…

高能物理 - 唯象学 · 物理学 2008-11-26 O. Felix , A. Mondragon , M. Mondragon , E. Peinado

I report the analysis performed on fermion masses and mixing, including neutrino mixing, within the context of a model with hierarchical radiative mass generation mechanism for light charged fermions, mediated by exotic scalar particles at…

高能物理 - 唯象学 · 物理学 2008-11-26 Albino Hernandez-Galeana

We study a neutrino mass model based on $S_4$ flavor symmetry which accommodates lepton mass, mixing with non-zero $\theta_{13}$ and CP violation phase. The spontaneous symmetry breaking in the model is imposed to obtain the realistic…

高能物理 - 唯象学 · 物理学 2016-04-20 V. V. Vien

We discuss the possibility of flavor symmetries to explain the pattern of charged lepton and neutrino masses and mixing angles. We emphasize what are the obstacles for the generation of an almost maximal atmospheric mixing and what are the…

高能物理 - 唯象学 · 物理学 2014-11-17 Shao-Long Chen , Michele Frigerio , Ernest Ma

We consider a supersymmetric model where the neutrino mass matrix arises from bilinear and trilinear R-parity violation, both restricted by a $Z_3$ flavor symmetry. Assuming flavor blind soft supersymmetry (SUSY) breaking conditions,…

高能物理 - 唯象学 · 物理学 2013-05-30 E. Peinado , A. Vicente

We derive formulae for neutrino masses and mixing angles in a type I seesaw framework with an underlying A4 flavor symmetry. In particular, the Majorana neutrino mass matrix includes contributions from an A4 triplet, 1, 1', and 1" flavon…

高能物理 - 唯象学 · 物理学 2013-02-22 Mu-Chun Chen , Jinrui Huang , Jon-Michael O'Bryan , Alexander M. Wijangco , Felix Yu

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

The hierarchy $\Delta m^2_{atm} \gg \Delta m^2_\odot$ and the large $\theta_{23}$ mixing angle, as suggested by neutrino oscillation experiments, can be accounted for by a variety of lepton flavour models. A dichotomy emerges: i) Models…

高能物理 - 唯象学 · 物理学 2007-05-23 Riccardo Barbieri

Lepton mixing can originate from the breaking of a flavor symmetry in different ways in the neutrino and the charged lepton sector. We propose an extension of this framework which allows to connect the mixing parameters with masses, and…

高能物理 - 唯象学 · 物理学 2013-11-27 D. Hernandez , A. Yu. Smirnov

Recently Babu, Ma and Valle proposed a model of quark and lepton mixing based on $A_4$ symmetry. Within this model the lepton and slepton mixings are intimately related. We perform a numerical study in order to derive the slepton masses and…

高能物理 - 唯象学 · 物理学 2010-04-06 M. Hirsch , J. C. Romao , S. Skadhauge , J. W. F. Valle , A. Villanova del Moral

The PMNS neutrino mixing matrix is given, in general, by the product of two unitary matrices associated with the diagonalization of the charged lepton and neutrino mass matrices, respectively. Assuming that the active flavor neutrinos…

高能物理 - 唯象学 · 物理学 2008-11-26 S. T. Petcov , W. Rodejohann