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We study the possibility of simultaneously addressing neutrino phenomenology and the dark matter in the framework of inverse seesaw. The model is the extension of the standard model by the addition of two right handed neutrinos and three…

高能物理 - 唯象学 · 物理学 2020-02-19 Nayana Gautam , Mrinal Kumar Das

We present a TeV scale seesaw mechanism for exploring the dark matter and neutrino phenomenology in the light of recent neutrino and cosmology data. A different realization of the Inverse seesaw(ISS) mechanism with $A_{4}$ flavor symmetry…

高能物理 - 唯象学 · 物理学 2016-10-20 Ananya Mukherjee , Mrinal Kumar Das

In this paper, we present a systematic investigation on simple inverse seesaw models for neutrino masses and flavor mixing based on the modular $S^{}_4$ symmetry. Two right-handed neutrinos and three extra fermion singlets are introduced to…

高能物理 - 唯象学 · 物理学 2021-10-01 Xinyi Zhang , Shun Zhou

In this paper we present a scenario where the stability of dark matter and the phenomenology of neutrinos are related by the spontaneous breaking of a non-Abelian flavor symmetry. In this scenario the breaking is done at the seesaw scale,…

高能物理 - 唯象学 · 物理学 2016-09-16 J. M. Lamprea , E. Peinado

We study $S_{4}$ flavor symmetric inverse seesaw model which has the possibility of simultaneously addressing neutrino phenomenology, dark matter (DM) and baryon asymmetry of the universe (BAU) through leptogenesis. The model is the…

高能物理 - 唯象学 · 物理学 2021-09-01 Nayana Gautam , Mrinal Kumar Das

We present a model constructed within a non-supersymmetric framework capable of explaining both current neutrino oscillation data and the observed dark matter relic abundance. In this study, the Yukawa couplings are expressed as…

高能物理 - 唯象学 · 物理学 2025-09-03 Bhabana Kumar , Mrinal Kumar Das

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

We investigate neutrino mass model based on $A_4$ discrete flavor symmetry in type-I+II seesaw framework. The model has imperative predictions for neutrino masses, mixing and $CP$ violation testable in the current and upcoming neutrino…

高能物理 - 唯象学 · 物理学 2019-07-29 Surender Verma , Monal Kashav , Shankita Bhardwaj

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 propose a minimal extension of the Standard Model with right-handed neutrinos, governed by a non-holomorphic $A_{4}$ modular flavor symmetry. Within this model framework, the light neutrino masses are generated via the popular type-I…

高能物理 - 唯象学 · 物理学 2026-02-13 Swaraj Kumar Nanda , Maibam Ricky Devi , Sudhanwa Patra

We present a unified framework for neutrino masses, baryogenesis, and dark matter based on a modular $S_4$ symmetry combined with a type-III seesaw mechanism. All Yukawa couplings, CP phases, and flavor textures originate from a single…

高能物理 - 唯象学 · 物理学 2026-02-04 Abhishek , V. Suryanarayana Mummidi

To understand the observed pattern of neutrino masses and mixing as well as to account for the dark matter we propose a hybrid scoto-seesaw model based on the $A_4$ discrete flavor symmetry. In this setup, including at least two heavy…

高能物理 - 唯象学 · 物理学 2022-11-30 Joy Ganguly , Janusz Gluza , Biswajit Karmakar

We construct a flavor symmetry model based on the tetrahedral group A_4 in which the right-handed neutrinos from the seesaw mechanism can be both keV warm dark matter particles and eV-scale sterile neutrinos. This is achieved by giving the…

高能物理 - 唯象学 · 物理学 2012-02-01 James Barry , Werner Rodejohann , He Zhang

A new idea for neutrino mass was proposed recently, where its smallness is not due to the seesaw mechanism, i.e. not inversely proportional to some large mass scale. It comes from a one-loop mechanism with dark matter in the loop consisting…

高能物理 - 唯象学 · 物理学 2013-06-06 Subhaditya Bhattacharya , Ernest Ma , Alexander Natale , Ahmed Rashed

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

We revisit the discrete dark matter model with $A_4$ flavor symmetry originally introduced by M.Hirsch {\it et.al}. We show that radiative corrections can lead to non-zero $\theta_{13}$ and non-zero mass for the lightest neutrino. We find…

高能物理 - 唯象学 · 物理学 2015-06-19 Yuta Hamada , Tatsuo Kobayashi , Atsushi Ogasahara , Yuji Omura , Fumihiro Takayama , Daiki Yasuhara

We propose a hybrid scoto-seesaw model based on the $A_4$ non-Abelian discrete flavor symmetry. Light neutrino masses come from the tree-level type-I seesaw mechanism and from the one-loop scotogenic contribution accommodating viable dark…

高能物理 - 唯象学 · 物理学 2024-07-09 Joy Ganguly , Janusz Gluza , Biswajit Karmakar , Satyabrata Mahapatra

A theoretical framework based on a spontaneously broken $Z_4$ symmetry is proposed to simultaneously explain neutrino mass generation via the inverse seesaw mechanism and dark matter (DM) production through a freeze-in scenario. This work…

高能物理 - 唯象学 · 物理学 2025-09-30 Ziye Wang , Yakefu Reyimuaji , Nijiati Yalikun

We propose a hybrid seesaw model based on $A_{4}$ flavor symmetry, which generates a large hierarchical flavor structure. In our model, tree-level and one-loop seesaw mechanisms predict different flavor structures in the neutrino mass…

高能物理 - 唯象学 · 物理学 2021-03-10 Mayumi Aoki , Daiki Kaneko

We build a highly predictive 3-3-1 model, where the field content is extended by including several $SU(3)_{L}$ scalar singlets and six right handed Majorana neutrinos. In our model the $SU(3)_{C}\times SU\left( 3\right) _{L}\times U\left(…

高能物理 - 唯象学 · 物理学 2019-05-24 A. E. Cárcamo Hernández , H. N. Long
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