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相关论文: Radiative Scaling Neutrino Mass with $A_4$ Symmetr…

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A new and radical scenario of the simple 2006 model of radiative neutrino mass is proposed, where there is no seesaw mechanism, i.e. neutrino masses are not inversely proportional to some large mass scale, contrary to the prevalent…

高能物理 - 唯象学 · 物理学 2015-06-05 Ernest Ma

The hierarchy in scale between atmospheric and solar neutrino mass splittings is investigated through two distinct neutrino mass mechanisms, from tree- and one-loop-level contributions. We demonstrate that the minimal discrete dark matter…

高能物理 - 唯象学 · 物理学 2023-06-16 Cesar Bonilla , Johannes Herms , Omar Medina , Eduardo Peinado

A new mechanism for generating neutrino masses without a high-energy mass scale is proposed. The mechanism needs a fundamental mass scale M in the 100-1000 TeV region and a minimal field content beyond the Standard Model one containing a…

高能物理 - 唯象学 · 物理学 2007-05-23 Emilian Dudas , Carlos A. Savoy

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 extension of the Standard Model with an inert scalar doublet, three right-handed neutrinos, and singlet scalar fields, $\varphi$ and $S$. In this model, neutrino masses are zero in the limit of the unbroken $Z_4$ discrete…

高能物理 - 唯象学 · 物理学 2025-07-18 Jongkuk Kim , Seong-Sik Kim , Hyun Min Lee , Rojalin Padhan

A new and novel idea for a predictive neutrino mass matrix is presented, using the non-Abelian discrete symmetry A(4) and the seesaw mechanism with only two heavy neutral fermion singlets. Given the components of the one necessarily…

高能物理 - 唯象学 · 物理学 2015-06-11 Ernest Ma

We consider the radiative generation of neutrino mass through the interactions of neutrinos with MeV dark matter. We construct a realistic renormalizable model with one scalar doublet and one complex singlet together with three light…

高能物理 - 唯象学 · 物理学 2016-07-15 Abdesslam Arhrib , Céline Bœhm , Ernest Ma , Tzu-Chiang Yuan

We explore a possible explanation for the hierarchy in scale between the atmospheric and solar neutrino mass differences ($\lvert \Delta m^{2}_{31} \rvert$, and $\Delta m^{2}_{21}$) through the presence of two distinct neutrino mass…

高能物理 - 唯象学 · 物理学 2023-02-20 Cesar Bonilla , Johannes Herms , Omar Medina , Eduardo Peinado

We propose a unique lepton mixing scheme and its association with an exact hierarchy-philic neutrino mass matrix texture in the light of Type-I+Type-II seesaw mechanism under the framework of $A_4 \times Z_{10}$ discrete flavour symmetry.…

高能物理 - 唯象学 · 物理学 2024-07-24 Manash Dey , Subhankar Roy

In this paper, we present a model based on $A_4$ discrete flavor symmetry implementing inverse and type-II seesaw mechanisms to have LHC accessible TeV scale right-handed neutrino mass and texture one-zero in the resulting Majorana neutrino…

高能物理 - 唯象学 · 物理学 2021-10-07 Rishu Verma , Monal Kashav , Surender Verma , B. C. Chauhan

The four light neutrino scenario, which explains the atmosphere, solar and LSND neutrino experiments, is studied in the framework of the seesaw mechanism. By taking both the Dirac and Majorana mass matrix of neutrinos to be singular, the…

高能物理 - 唯象学 · 物理学 2009-10-31 Chun Liu , Jeonghyeon Song

We propose a unified solution with $Z_4$ discrete symmetry for small neutrino masses and stability of dark matter. The Standard Model is extended with an inert doublet scalar, a dark singlet scalar, a spurion scalar and right-handed…

高能物理 - 唯象学 · 物理学 2025-01-03 Jongkuk Kim , Seong-Sik Kim , Hyun Min Lee , Rojalin Padhan

In the context of the non-Abelian discrete symmetry $A_4$, the neutrino mass matrix has been studied extensively. A brief update is presented to focus on the conceptual shift from tribimaximal mixing ($\theta_{13} = 0$, $\theta_{23} =…

高能物理 - 唯象学 · 物理学 2015-12-02 Ernest Ma

We study a model of neutrino and dark matter within the framework of a minimal extended seesaw. This framework is based on $A_4$ flavor symmetry along with the discrete $Z_4$ symmetry to stabilize the dark matter and construct desired mass…

高能物理 - 唯象学 · 物理学 2020-04-22 Pritam Das , Mrinal Kumar Das , Najimuddin Khan

A minimal extension of the standard model to naturally generate small neutrino masses and provide a dark matter candidate is proposed. The dark matter particle is part of a new scalar doublet field that plays a crucial role in radiatively…

高能物理 - 唯象学 · 物理学 2014-07-03 Michael Gustafsson , Jose Miguel No , Maximiliano A. Rivera

In a new application of the discrete non-Abelian symmetry A_4 using the canonical seesaw mechanism, a three-parameter form of the neutrino mass matrix is derived. It predicts the following mixing angles for neutrino oscillations:…

高能物理 - 唯象学 · 物理学 2009-11-11 Ernest Ma

We suggest a low-scale model based on $A_4\times Z_4 \times Z_2$ symmetry and a global lepton number $U(1)_L$ symmetry capable of generating the current neutrino data. The neutrino mass smallness is reproduced by the linear seesaw…

高能物理 - 唯象学 · 物理学 2023-02-08 V. V. Vien , H. N. Long

We propose an extension of the Standard Model (SM) for radiative neutrino mass by introducing a dark $U(1)_D$ gauge symmetry. The kinetic mixing between the SM gauges and the dark $U(1)_D$ gauge arises at 1-loop mediated by new inert scalar…

高能物理 - 唯象学 · 物理学 2021-04-20 Arnab Dasgupta , Sin Kyu Kang , Myeonghun Park

The simplest possibility to generate small Majorana neutrino masses is the seesaw mechanism. However, the smallness of the observed neutrino masses can also be understood, if neutrino masses are generated by higher-dimensional operators…

高能物理 - 唯象学 · 物理学 2020-05-20 Ricardo Cepedello , Renato Fonseca , Martin Hirsch

We propose an A_4 flavor-symmetric SU(3)xSU(2)xU(1) seesaw model where lepton number is broken spontaneously. A consistent two-zero texture pattern of neutrino masses and mixing emerges from the interplay of type-I and type-II seesaw…

高能物理 - 唯象学 · 物理学 2014-11-21 J. N. Esteves , F. R. Joaquim , A. S. Joshipura , J. C. Romao , M. A. Tortola , J. W. F. Valle
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