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相关论文: Stability of dark matter from the D4xZ2 flavor gro…

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I comment on the proposal that the stability of dark matter may be due to an unbroken Z_2 symmetry contained in the partially broken lepton flavour symmetry group. I remark that (1) there is no Z_2 symmetry apparent in the lepton mass…

高能物理 - 唯象学 · 物理学 2015-05-30 L. Lavoura

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 propose a new motivation for the stability of dark matter (DM). We suggest that the same non-abelian discrete flavor symmetry which accounts for the observed pattern of neutrino oscillations, spontaneously breaks to a Z2 subgroup which…

高能物理 - 唯象学 · 物理学 2010-12-24 M. Hirsch , S. Morisi , E. Peinado , J. W. F. Valle

We present a mechanism for the dark matter stability in the framework of a non-Abelian avour symmetry renormalizable model. The same non-abelian discrete avor symmetry which accounts for the observed pattern of neutrino oscillations,…

高能物理 - 唯象学 · 物理学 2015-06-03 E. Peinado

In a simple framework which naturally incorporates dark matter stability and neutrino phenomenology, we compute all the possible texture zeros which arise when the non-abelian flavor symmetry A4 is spontaneously broken to Z2. As a result,…

高能物理 - 唯象学 · 物理学 2019-04-01 Leon M. G. de la Vega , R. Ferro-Hernandez , E. Peinado

We consider a model in which dark matter is stable as it is charged under a Z2 symmetry that is residual after an A4 flavour symmetry is broken. We consider the possibility to generate the quark masses by charging the quarks appropriately…

高能物理 - 唯象学 · 物理学 2015-03-19 Reinier de Adelhart Toorop , Federica Bazzocchi , Stefano Morisi

Dark Matter stability can be achieved through a partial breaking of a flavor symmetry. In this framework we propose a type-II seesaw model where left-handed matter transforms nontrivially under the flavor group Delta(54), providing…

高能物理 - 唯象学 · 物理学 2015-06-04 M. S. Boucenna , S. Morisi , E. Peinado , Y. Shimizu , J. W. F. Valle

We propose that dark matter is stable as a consequence of an accidental Z2 that results from a flavour-symmetry group which is the double-cover group of the symmetry group of one of the regular geometric solids. Although model-dependent,…

高能物理 - 唯象学 · 物理学 2015-06-05 L. Lavoura , S. Morisi , J. W. F. Valle

Recent analysis of spontaneous breaking of SU(2) as a continuous gauged flavor symmetry to non-abelian discrete group Q4 as a residual symmetry motivates its consideration as a group for stabilizing dark matter. We determine the region of…

高能物理 - 唯象学 · 物理学 2012-12-06 I. Lovrekovic

We present a scenario where the stability of dark matter and the phenomenology of neutrinos are related by the breaking of a flavour symmetry. We propose two models based on this idea for which we have obtained interesting neutrino and dark…

高能物理 - 唯象学 · 物理学 2017-10-25 J. M. Lamprea

We consider the possibility that dark matter is stabilised by a discrete $Z_2$ symmetry which arises from a subgroup of a $U(1)'$ gauge symmetry, spontaneously broken by integer charged scalars, and under which the chiral quarks and leptons…

高能物理 - 唯象学 · 物理学 2022-01-05 Bowen Fu , Stephen F. King

We propose to relate dark matter stability to the possible Dirac nature of neutrinos. The idea is illustrated in a simple scheme where small Dirac neutrino masses arise from a type-I seesaw mechanism as a result of a $Z_4$ discrete lepton…

高能物理 - 唯象学 · 物理学 2017-12-05 Salvador Centelles Chuliá

We propose a model based on modular $A_4$ symmetry containing a dark matter candidate, realizing radiatively induced neutrino mass at one-loop level. One finds that stability of dark matter candidate can be assured by nonzero value of…

高能物理 - 唯象学 · 物理学 2019-08-07 Takaaki Nomura , Hiroshi Okada

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 investigate scenarios in which dark matter is stabilized by an abelian Z_N discrete gauge symmetry. Models are surveyed according to symmetries and matter content. Multi-component dark matter arises when N is not prime and Z_N contains…

高能物理 - 唯象学 · 物理学 2011-02-18 Brian Batell

We present the Discrete Dark Matter mechanism (DDM) which consist on the stability of the dark matter from a spontaneous breaking of a flavor symmetry group into one of its subgroups. Here we present the inclusion of the quarks on this…

高能物理 - 唯象学 · 物理学 2012-10-26 E. Peinado

We investigate the phenomenology of flavored dark matter (DM). DM stability is guaranteed by an accidental ${\mathcal Z}_3$ symmetry, a subgroup of the standard model (SM) flavor group that is not broken by the SM Yukawa interactions. We…

高能物理 - 唯象学 · 物理学 2016-01-27 Fady Bishara , Admir Greljo , Jernej F. Kamenik , Emmanuel Stamou , Jure Zupan

The stability of dark matter is normally achieved by imposing extra symmetries beyond those of the Standard Model of Particle Physics. In this paper we present a framework where the dark matter stability emerges as a consequence of the…

高能物理 - 唯象学 · 物理学 2014-09-17 Oscar Cata , Alejandro Ibarra

Apparent regularities in fermion masses and mixings are often associated with physics at a high flavor scale, especially in the context of discrete flavor symmetries. One of the main reasons for that is that the correct vacuum alignment…

高能物理 - 唯象学 · 物理学 2013-03-14 Martin Holthausen , Manfred Lindner , Michael A. Schmidt

We present a Majorana scotogenic-like loop framework in which neutrino mass generation and dark matter stability are intrinsically connected to the breaking of the discrete flavor symmetry $A_4$. This breaking leads to the emergence of the…

高能物理 - 唯象学 · 物理学 2025-11-25 Ranjeet Kumar , Hemant Kumar Prajapati , Rahul Srivastava , Sushant Yadav
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