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Finite discrete subgroups of $U(3)$ as possible flavour symmetries $G_f$ for a massless neutrinos with predictive mixing angles are studied. This is done by assuming that a residual symmetry $S_\nu$ appropriate for describing a massless…

高能物理 - 唯象学 · 物理学 2014-04-07 Anjan S. Joshipura , Ketan M. Patel

We propose a Standard Model extension with underlying A4 flavour symmetry where small Dirac neutrino masses arise from a Type-II seesaw mechanism. The model predicts the "golden" flavour-dependent bottom-tau mass relation, requires an…

高能物理 - 唯象学 · 物理学 2018-02-21 Cesar Bonilla , J. M. Lamprea , Eduardo Peinado , Jose W. F. Valle

We study a number of models, based on a non-Abelian discrete group, that successfully reproduce the simple and predictive Yukawa textures usually associated with U(2) theories of flavor. These models allow for solutions to the solar and…

高能物理 - 唯象学 · 物理学 2008-11-26 Alfredo Aranda , Christopher D. Carone , Richard F. Lebed

The Type I, II and hybrid (I+II) seesaw mechanism, which explain why neutrinos are especially light, are consequences of the left-right symmetric model (LRSM). They can be classified by the ranges of parameters of LRSM. We show that a…

高能物理 - 唯象学 · 物理学 2009-03-04 M. J. Luo , Q. Y. Liu

Experiments on neutrino oscillations have uncovered several small parameters, $\theta_{13}$ being a prominent one. Others are the solar mass splitting {\em vis-\`{a}-vis} the atmospheric one and the deviation of $\theta_{23}$ from maximal…

高能物理 - 唯象学 · 物理学 2015-05-27 Soumita Pramanick , Amitava Raychaudhuri

We introduce the idea of Form Dominance in the (type I) see-saw mechanism, according to which a particular right-handed neutrino mass eigenstate is associated with a particular physical neutrino mass eigenstate, leading to a form…

高能物理 - 唯象学 · 物理学 2010-05-12 Mu-Chun Chen , Stephen F. King

What we call the Anti-GUT model is extended a bit to include also right-handed neutrinos and thus make use of the see-saw mechanism for neutrino masses. This model consists in assigning gauge quantum numbers to the known Weyl fermions and…

高能物理 - 唯象学 · 物理学 2009-10-31 C. D. Froggatt , H. B. Nielsen , Y. Takanishi

We present an S$_4$ flavour symmetric model within a minimal seesaw framework resulting in mass matrices that leads to TM$_1$ mixing. Minimal seesaw is realized by adding two right-handed neutrinos to the Standard Model. The model predicts…

高能物理 - 唯象学 · 物理学 2021-12-22 Bikash Thapa , Ng. K. Francis

We present a $SU(5)\times U(1)_F$ supersymmetric model for neutrino masses and mixings that implements the seesaw mechanism by means of the heavy SU(2) singlets and triplets states contained in three adjoints of SU(5). We discuss how…

高能物理 - 唯象学 · 物理学 2015-05-30 Enrico Nardi , Diego Restrepo , Mauricio Velasquez

Right-handed neutrinos $N$ are introduced to explain the origin of the tiny neutrino masses via the seesaw mechanism. Required by relatively large Yukawa coupling and leptogenesis, masses of right-handed neutrinos are beyond $10^{9}$ GeV.…

高能物理 - 唯象学 · 物理学 2025-06-23 Cai-Xia Yang , Zhi-Long Han , Fei Huang , Yi Jin , Honglei Li

We point out that the minimal seesaw model can provide a natural framework to accommodate tiny neutrino masses, while its experimental testability and notable predictiveness are still maintained. This possibility is based on the observation…

高能物理 - 唯象学 · 物理学 2010-05-12 He Zhang , Shun Zhou

The measured values for the mixture angles in neutrino oscillations suggest the existence of a symmetry of interchange of flavor between muon and tau neutrinos. Using this symmetry we analyzed the minimal seesaw model for neutrino masses,…

高能物理 - 唯象学 · 物理学 2008-01-22 Daniel Wegman Ostrosky

We construct a neutrino mass model based on the flavour symmetry group $A_4\times C_4 \times C_6 \times C_2$ which accommodates a light sterile neutrino in the minimal extended seesaw (MES) scheme. Besides the flavour symmetry, we introduce…

高能物理 - 唯象学 · 物理学 2020-11-04 R. Krishnan , Ananya Mukherjee , Srubabati Goswami

In this paper, we construct a model with the help of modular symmetry in the framework of minimal inverse seesaw [ISS(2,3)]. We have used $\Gamma(3)$ modular group which is isomorphic to non-Abelian discrete symmetry group $A_4$. In this…

高能物理 - 唯象学 · 物理学 2023-05-03 Jotin Gogoi , Nayana Gautam , Mrinal Kumar Das

Stimulated by the recent development of the ``universal seesaw mass matrix model", an application of the model to the neutrino mass matrix is investigated: For the charged lepton and down-quark sectors, the model explains the smallness of…

高能物理 - 唯象学 · 物理学 2007-05-23 Yoshio Koide

The presently available information on neutrino oscillations can be used to tightly constrain the light neutrino mass matrix $m_\n$ under the assumption that the three known neutrinos provide explanation of the solar and atmospheric…

高能物理 - 唯象学 · 物理学 2007-05-23 Anjan S. Joshipura , Emmanuel A. Paschos

We consider an extension of the Standard Model with three right-handed (RH) neutrinos and a Dirac pair of extra sterile neutrinos, odd under a discrete $Z_2$ symmetry, in order to have left-right symmetry in the neutrino content and obtain…

高能物理 - 唯象学 · 物理学 2021-08-11 Ernesto A. Matute

We find a realization of the $Z_2$-symmetry in the neutrino mass matrix which expresses a rotation of the $\mu-\tau$ symmetry and is able to impose a generic smallest mixing angle, in contrast to a zero-value predicted by the usual…

高能物理 - 唯象学 · 物理学 2017-07-12 E. I. Lashin , N. Chamoun , C. Hamzaoui , S. Nasri

Fermion masses and mixing matrices can be described in terms of spontaneously broken (global or gauge) flavor symmetries. We propose a little-Higgs inspired scenario in which an SU(2)xU(1) gauge flavor symmetry is spontaneously (and…

高能物理 - 唯象学 · 物理学 2009-11-10 F. Bazzocchi , S. Bertolini , M. Fabbrichesi , M. Piai

We show that the assumption of type II seesaw mechanism for small neutrino masses coupled with $b-\tau$ mass unification in a minimal SUSY SO(10) model leads not only to a natural understanding of large atmospheric mixing angle…

高能物理 - 唯象学 · 物理学 2008-11-26 H. S. Goh , R. N. Mohapatra , Siew-Phang Ng