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相关论文: Unifying the flavor origin of dark matter with lep…

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We propose a minimal extension of the standard model by including a $U(1)$ flavor symmetry to establish a correlation between the relic abundance of dark matter, measured by WMAP and PLANCK satellite experiments and non-zero value of $\sin…

高能物理 - 唯象学 · 物理学 2017-06-07 Subhaditya Bhattacharya , Biswajit Karmakar , Narendra Sahu , Arunansu Sil

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

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 study a new flavor symmetric model with non-Abelian discrete symmetry T_{13}. The T_{13} group is isomorphic to Z_{13} \rtimes Z_3, and it is the minimal group having two complex triplets as the irreducible representations. We show that…

高能物理 - 唯象学 · 物理学 2011-08-04 Yuji Kajiyama , Hiroshi Okada

The fundamental issue of the origin of mass for all quarks and leptons (including Majorana neutrinos) is linked to dark matter, odd under an exactly conserved Z(2) symmetry which may or may not be derivable from an U(1) gauge symmetry. The…

高能物理 - 唯象学 · 物理学 2015-06-17 Ernest Ma

We provide an $A_4$ based flavor symmetric scenario to accommodate the inverse seesaw mechanism for explaining light neutrino masses and mixing. We find that the lepton mixing, in particular the tri-bimaximal mixing pattern and its…

高能物理 - 唯象学 · 物理学 2017-08-07 Biswajit Karmakar , Arunansu Sil

We propose a model of asymmetric dark matter (DM) where the dark sector is an identical copy of both forces and matter of the standard model (SM) as in the mirror universe models discussed in literature. In addition to being connected by…

高能物理 - 唯象学 · 物理学 2010-04-08 Haipeng An , Shao-Long Chen , Rabindra N. Mohapatra , Yue Zhang

We study an inverse seesaw model of neutrino mass within the framework of $S_4$ flavour symmetry from the requirement of generating non-zero reactor mixing angle $\theta_{13}$ along with correct dark matter relic abundance. The leading…

高能物理 - 唯象学 · 物理学 2017-07-19 Ananya Mukherjee , Debasish Borah , Mrinal Kumar Das

We propose a new scenario in a radiative seesaw model based on A_4 flavor symmetry. In this model, we explore a possibility of linking non-zero \theta_{13} to dark matter. And we analyze the lepton sector to predict the observed neutrinos…

高能物理 - 唯象学 · 物理学 2015-06-03 Y. H. Ahn , Hiroshi Okada

Recent observations for a non-zero $\theta_{13}$ have come from various experiments. We study a model of lepton mixing with a 2-3 flavor symmetry to accommodate the sizable $\theta_{13}$ measurement. In this work, we derive deviations from…

高能物理 - 唯象学 · 物理学 2015-03-19 Ahmed Rashed

We propose an $A_4$ extension of the Standard Model with a Lepton Quarticity symmetry correlating dark matter stability with the Dirac nature of neutrinos. The flavor symmetry predicts (i) a generalized bottom-tau mass relation involving…

高能物理 - 唯象学 · 物理学 2017-09-13 Salvador Centelles Chuliá , Rahul Srivastava , José W. F. Valle

We examine the sterile neutrino dark matter production in the primordial plasma with lepton asymmetry unequally distributed over different neutrino flavors. We argue that with the specific flavor fractions, one can mitigate limits from the…

高能物理 - 唯象学 · 物理学 2025-07-29 Dmitry Gorbunov , Dmitry Kalashnikov , George Krugan

In this work we discuss the neutrino phenomenology in a $\Delta(54)$ discrete flavor symmetry and evaluate the relic abundance of dark matter (DM) and active neutrino-DM mixing angle considering various cosmological constraints. We…

高能物理 - 唯象学 · 物理学 2024-07-09 Hrishi Bora , Ng. K. Francis , Shawan Kumar Jha

In flavored dark matter models, dark matter can scatter off of nuclei through Higgs and photon exchange, both of which can arise from renormalizable interactions and individually lead to strong constraints from direct detection. While these…

高能物理 - 唯象学 · 物理学 2015-03-05 Ali Hamze , Can Kilic , Jason Koeller , Cynthia Trendafilova , Jiang-Hao Yu

I proposed a unified model of particle physic and cosmology in \cite {1}, which can simultaneously account for these origin of the inflation, dark energy, dark matter, neutrino mass and baryon asymmetry. I here focus on the fermion flavor…

综合物理 · 物理学 2025-10-23 Wei-Min Yang

In this paper, we present a model which attempts to unify a new dark sector force with a local $SU(3)$ flavor symmetry. Dark Matter (DM) and its potential interactions with the Standard Model (SM) continue to present a rich framework for…

高能物理 - 唯象学 · 物理学 2022-01-10 George N. Wojcik , Thomas G. Rizzo

We investigate a model in which Dark Matter is stabilized by means of a Z2 parity that results from the same non-abelian discrete flavor symmetry which accounts for the observed pattern of neutrino mixing. In our A4 example the standard…

高能物理 - 唯象学 · 物理学 2015-03-17 M. S. Boucenna , M. Hirsch , S. Morisi , E. Peinado , M. Taoso , J. W. F. Valle

We explore scalar dark matter that is part of a lepton flavor triplet satisfying symmetry requirements under the hypothesis of minimal flavor violation. Beyond the standard model, the theory contains in addition three right-handed neutrinos…

高能物理 - 唯象学 · 物理学 2015-05-06 Chao-Jung Lee , Jusak Tandean

The origin of neutrino masses and the nature of dark matter are two of the most pressing open questions of the modern astro-particle physics. We consider here the possibility that these two problems are related, and review some theoretical…

高能物理 - 唯象学 · 物理学 2015-01-20 Massimiliano Lattanzi , Roberto A. Lineros , Marco Taoso

In the context of the type-I seesaw mechanism, it is known that $\theta_{13}$ is zero and leptogenesis can not be realized if there exists a residual flavor symmetry resulting in the Tri-Bimaximal neutrino mixing pattern. We propose a…

高能物理 - 唯象学 · 物理学 2015-06-19 Wei-Chih Huang
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