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The seesaw mechanism of neutrino mass generation is analysed under the following assumptions: (1) minimal seesaw with no Higgs triplets, (2) hierarchical Dirac masses of neutrinos, (3) large lepton mixing primarily or solely due to the…

高能物理 - 唯象学 · 物理学 2008-11-26 E. Kh. Akhmedov

We consider the seesaw mechanism of neutrino mass generation in the light of our present knowledge of the neutrino masses and mixing. We analyse the seesaw mechanism constrained by the following assumptions: (1) minimal seesaw with no Higgs…

高能物理 - 唯象学 · 物理学 2008-11-26 E. Kh. Akhmedov , G. C. Branco , M. N. Rebelo

We present a quantitative study of the ability of models with different levels of hierarchy to reproduce the solar neutrino solutions, in particular the LA solution. As a flexible testing ground we consider models based on SU(5)xU(1)_F. In…

高能物理 - 唯象学 · 物理学 2009-11-07 Guido Altarelli , Ferruccio Feruglio , Isabella Masina

By inverting the seesaw formula we determine the heavy neutrino mass matrix. The impact on the baryogenesis via leptogenesis and the radiative lepton decays in supersymmetric models is described. Links to neutrinoless double beta decay are…

高能物理 - 唯象学 · 物理学 2009-11-10 D. Falcone

After summarizing neutrino oscillation results I discuss high and low-scale seesaw mechanisms, with or without supersymmetry, as well as recent attempts to understand the pattern of neutrino mixing from flavor symmetries. I also mention the…

高能物理 - 唯象学 · 物理学 2014-11-20 J. W. F. Valle

We provide a comprehensive analysis of the Type-I Seesaw family of neutrino mass models, including the conventional type-I seesaw and its low-scale variants, namely the linear and inverse seesaws. We establish that all these models…

高能物理 - 唯象学 · 物理学 2025-11-17 Salvador Centelles Chuliá , Antonio Herrero-Brocal , Avelino Vicente

We propose a flavour model based on an $A_4$ symmetry combined with a type-II seesaw mechanism for neutrino mass generation. The resulting neutrino mass matrix obeys a sum rule that, together with the measured mass-squared differences,…

高能物理 - 唯象学 · 物理学 2026-03-16 Salvador Centelles Chuliá , Ranjeet Kumar

We investigate Type-I Seesaw models where the right-handed neutrino masses are dynamically generated by strong interactions. Using horizontal gauge symmetry as the source of strong dynamics, a nontrivial flavor structure can also be…

高能物理 - 唯象学 · 物理学 2024-04-19 Yi Chung

We study neutrino mass generation within the framework of non-holomorphic modular symmetry proposed by Qu and Ding. In this formalism, neutrino masses are generated via the Type-I seesaw mechanism, where the Yukawa couplings depend on…

高能物理 - 唯象学 · 物理学 2026-04-21 Cheshta , Priya , Suneel Dutt , B. C. Chauhan

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

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

We derive the lower bound on absolute scale of lightest neutrino mass for normal hierarchy and inverted hierarchy pattern of light neutrinos by studying the new physics contributions to charged lepton flavour violating decays and…

高能物理 - 唯象学 · 物理学 2022-07-25 Prativa Pritimita , Urjit A. Yajnik , Nitali Dash , Sudhanwa Patra

We consider numerical fits to non-supersymmetric $\mathrm{SO}(10)$-based models in which neutrino mass is generated by the type-I or type-II seesaw mechanism or a combination of both. The fits are performed with a sophisticated top-down…

高能物理 - 唯象学 · 物理学 2019-06-20 Tommy Ohlsson , Marcus Pernow

In the type-I seesaw model the size of mixing between light and heavy neutrinos, nu and N, respectively, is of order the square root of their mass ratio, (m_nu/m_N)^(1/2), with only one generation of the neutrinos. Since the light-neutrino…

高能物理 - 唯象学 · 物理学 2010-06-21 Xiao-Gang He , Sechul Oh , Jusak Tandean , Chung-Cheng Wen

The problem of neutrino masses and mixing angles is analysed in a class of supersymmetric grand unified models, with SO(10) gauge symmetry and global U(2) flavour symmetry. Adopting the seesaw mechanism for the generation of the neutrino…

高能物理 - 唯象学 · 物理学 2009-10-30 G. Costa , E. Lunghi

We present a comparative analysis of neutrino models based on a broad class of low scale seesaw mechanisms, viz., type II, inverse (ISS) and linear seesaw (LSS) mechanisms that are used to realize the tiny masses of neutrino. In particular,…

高能物理 - 唯象学 · 物理学 2021-12-23 Maibam Ricky Devi , Kalpana Bora

We consider the scenario in which neutrino data are explained by the interplay of type I and II seesaw terms in the Majorana neutrino mass matrix ${\cal M}_\nu = {\cal M}_L - {\cal M}_D {\cal M}_R^{-1} {\cal M}_D^T$. We construct a…

高能物理 - 唯象学 · 物理学 2011-05-05 Shao-Long Chen , Michele Frigerio , Ernest Ma

We consider seesaw type-I models including at least one (mostly-)sterile neutrino with mass at the eV scale. Three distinct situations are found, where the presence of light extra neutrinos is naturally justified by an approximately…

高能物理 - 唯象学 · 物理学 2020-08-26 G. C. Branco , J. T. Penedo , Pedro M. F. Pereira , M. N. Rebelo , J. I. Silva-Marcos

Seesaw mechanism provides a natural explanation of light neutrino masses through suppression of heavy seesaw scale. In inverse seesaw models the seesaw scale can be much lower than that in the usual seesaw models. If terms inducing seesaw…

高能物理 - 唯象学 · 物理学 2015-06-05 Gang Guo , Xiao-Gang He , Guan-Nan Li

Seesaw mechanism appears to be the simplest and most appealing way to understand small neutrino masses observed in recent experiments. It introduces three right handed neutrinos with heavy masses to the standard model, with at least one…

高能物理 - 唯象学 · 物理学 2014-11-18 R. N. Mohapatra