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Related papers: Neutrino Masses in E_6 Unification

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I demonstrate that neutrino large mixing between $\nu_\mu$ and $\nu_\tau$ are naturally reproduced using a novel mechanism called `E-twisting'in a supersymmetric $E_6$ grand unification model. This model explains all the characteristic…

High Energy Physics - Phenomenology · Physics 2007-05-23 Masako Bando

Motivated by the Super-Kamiokande data, we revisit models with U(1) symmetries and discuss the origin of neutrino masses and mixings in such theories. We show that, in models with just three light neutrinos and a hierarchy of neutrino…

High Energy Physics - Phenomenology · Physics 2009-10-31 Smaragda Lola , Graham G. Ross

We study the generation of neutrino masses in the $SU(3)_W$ electroweak unified theory in $M_4\times S_1/(Z_2\times Z'_2)$ spacetime. By appropriate orbifolding, the bulk symmetry $SU(3)_W$ is broken into $SU(2)_L \times U(1)_Y$ at one of…

High Energy Physics - Phenomenology · Physics 2011-07-19 Chia-Hung V. Chang , We-Fu Chang , John N. Ng

We propose a model based on the $SU(5)$ grand unification with an extra $A_{4}\otimes Z_{2}\otimes Z_{2}^{\prime }\otimes Z_{2}^{\prime \prime}\otimes U\left( 1\right) _{f}$ flavor symmetry, which accounts for the pattern of the SM fermion…

High Energy Physics - Phenomenology · Physics 2015-06-19 Miguel D. Campos , A. E. Cárcamo Hernández , S. Kovalenko , Iván Schmidt , Erik Schumacher

We propose a supersymmetric extra U(1) model, which can generate small neutrino masses and necessary $\mu$ terms, simultaneously. Fields including quarks and leptons are embedded in three ${\bf 27}$s of $E_6$ in a different way among…

High Energy Physics - Phenomenology · Physics 2014-11-20 Daijiro Suematsu , Takashi Toma , Tetsuro Yoshida

Neutrino masses have been extensively studied in the context of discrete symmetries. A family permutation symmetry easily explains all neutrino oscillations and their mixing angles. However it is not obvious the embedding of such symmetry…

High Energy Physics - Phenomenology · Physics 2016-09-06 Francesco Caravaglios , Stefano Morisi

We present an $E_6$ Grand Unified model with a realistic pattern of fermion masses. All standard model fermions are unified in three fundamental 27-plets (i.e. supersymmetry is not invoked), which involve in addition right handed neutrinos…

High Energy Physics - Phenomenology · Physics 2009-11-10 Berthold Stech , Zurab Tavartkiladze

The combined requirements, of (i) a natural solution to the fermion mass hierarchy problem and (ii) an explanation of both the atmospheric and solar neutrino problems, lead to an essentially unique picture of neutrino masses and mixing…

High Energy Physics - Phenomenology · Physics 2009-10-30 C. D. Froggatt , M. Gibson , H. B. Nielsen

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…

High Energy Physics - Phenomenology · Physics 2008-11-26 Albino Hernandez-Galeana

Assuming three light neutrinos and the see-saw mechanism we present a semiquantitative model of fermion masses based on (SUSY) SU(5) and abelian horizontal charges. A good description of the observed pattern of quark and lepton masses is…

High Energy Physics - Phenomenology · Physics 2008-11-26 Guido Altarelli , Ferruccio Feruglio

Extensions of the Standard Model with additional U(1) symmetries can describe the hierarchy of fermion masses and mixing angles, including neutrinos. The neutrino masses and mixings are determined up to a discrete ambiguity corresponding to…

High Energy Physics - Phenomenology · Physics 2007-05-23 G. K. Leontaris , S. Lola

We discuss some models of neutrino masses and mixings in the context of fermion masses in Grand Unified Theories.

High Energy Physics - Phenomenology · Physics 2009-10-31 G. Altarelli

Superstring derived $\E$ models can accommodate small neutrino masses if a discrete symmetry is imposed which forbids tree level Dirac neutrino masses but allows for radiative mass generation. The only possible symmetries of this kind are…

High Energy Physics - Phenomenology · Physics 2009-09-25 Enrico Nardi

Within the framework of grand unified theories, we make full analysis of symmetric texture to see if such texture can reproduce large neutrino mixings, which have recently been confirmed by the observed solar and atmospheric neutrino…

High Energy Physics - Phenomenology · Physics 2009-11-10 Masako Bando , Midori Obara

We investigate a simple model of neutrino mass based on SU(3)_C X SU(3)_L X U(1)_X gauge unification. The Yukawa coupling of the model has automatic lepton-number symmetry which is broken only by the self-couplings of the Higgs boson. At…

High Energy Physics - Phenomenology · Physics 2008-11-26 Darwin Chang , Hoang Ngoc Long

One puzzle of neutrino masses and mixings is that they do not exhibit the kind of strong "hierarchy" that is found for the quarks and charged leptons. Neutrino mass ratios and mixing angles are not small. A possible reason for this is…

High Energy Physics - Phenomenology · Physics 2011-05-12 S. M. Barr

A natural solution to the fermion mass hierarchy problem suggests the existence of a partially conserved chiral symmetry. We show that this can lead to a reasonably natural solution to the solar and atmospheric neutrino problems without…

High Energy Physics - Phenomenology · Physics 2009-10-31 C. D. Froggatt , M. Gibson , H. B. Nielsen

The fermion mass problem is briefly reviewed. The observed hierarchy of quark and charged lepton masses strongly suggests the existence of an approximately conserved chiral flavour symmetry beyond the Standard Model. It is argued that in…

High Energy Physics - Phenomenology · Physics 2007-05-23 C. D. Froggatt

The idea of quark-lepton universality at high energies has recently been explored in unified theories based upon the quartification gauge group SU(3)^4. These schemes encompass a quark-lepton exchange symmetry that results upon the…

High Energy Physics - Phenomenology · Physics 2009-11-11 Alison Demaria , Catherine I. Low , Raymond R. Volkas

The atmospheric neutrino data imply large mixing between the $\nu_\mu$ and $\nu_\tau$ states, $\theta_{23} = (45\pm 12)^\circ$, while the MSW solution to the solar neutrino problem needs very small mixing angle $\theta_{12} = (2\pm…

High Energy Physics - Phenomenology · Physics 2010-02-03 Zurab Berezhiani , Anna Rossi
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