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The A4 x U(1) flavor model of He, Keum, and Volkas is extended to provide a minimal modification to tribimaximal mixing that accommodates a nonzero reactor angle theta13 ~ 0.1. The sequestering problem is circumvented by forbidding…

高能物理 - 唯象学 · 物理学 2013-01-15 Yoni BenTov , Xiao-Gang He , A. Zee

We study the modification of the Altarelli-Feruglio $A_4$ flavor symmetry model by adding three singlet flavons $\xi'$, $\xi''$ and $\rho$ and the model is augmented with extra $Z_2\times Z_2^ \prime$ symmetry to prevent the unwanted terms…

高能物理 - 唯象学 · 物理学 2023-02-28 Animesh Barman , Ng. K. Francis , Bikash Thapa , Ankur Nath

A grand unified $SU(5)$ theory is constructed with a hierarchical breaking of a $U(2)$ flavor symmetry. The small parameters of the squark and slepton mass matrices, necessary to solve the supersymmetric flavor-changing problem, and the…

高能物理 - 唯象学 · 物理学 2007-05-23 Riccardo Barbieri , Lawrence Hall

Flavour symmetries are fundamental tools in the search for an explanation to the flavour puzzle: fermion mass hierarchies, the neutrino mass ordering, the differences between the mixing matrices in the quark and lepton sector, can all find…

高能物理 - 唯象学 · 物理学 2014-11-12 Luca Merlo

We first time show that a common solution to dark matter and the flavor problem of the standard model can be obtained in the framework of the $\mathcal{Z}_{\rm N} \times \mathcal{Z}_{\rm M}$ flavor symmetry where the flavonic Goldstone…

高能物理 - 唯象学 · 物理学 2023-12-29 Gauhar Abbas , Rathin Adhikari , Eung Jin Chun

We propose a minimal $A_4$ flavor symmetric model, assisted by $Z_2 \times Z_3$ symmetry, which can naturally takes care of the appropriate lepton mixing and neutrino masses via Type-I seesaw. It turns out that the framework, originated due…

高能物理 - 唯象学 · 物理学 2022-01-05 Arghyajit Datta , Biswajit Karmakar , Arunansu Sil

Neutrino flavor mixing is explained within the recently proposed low-scale minimal linear seesaw model of neutrino mass generation, a variant of the standard linear seesaw led by a Dirac pair of extra sterile neutrinos which is odd under a…

高能物理 - 唯象学 · 物理学 2022-12-29 Ernesto A. Matute

Effective Supersymmetry is presented as a theory of physics above the electroweak scale which has significant theoretical advantages over both the standard model and the Minimal Supersymmetric Standard Model (MSSM). The theory is…

高能物理 - 唯象学 · 物理学 2009-10-28 A. G. Cohen , D. B. Kaplan , A. E. Nelson

We study general properties of attractors for tachyonic potential chameleon scalar-field model which possess cosmological scaling solutions. An analytic formulation is given to obtain fixed points with a discussion on their stability. The…

广义相对论与量子宇宙学 · 物理学 2015-05-28 H. Farajollahi , A. Salehi , F. Tayebi , A. Ravanpak

A modified neutrino mass model with five extra scalars is constructed using $A_{4}$ discrete symmetry group. The resultant mass matrix is able to give necessary deviation from Tribimaximal mixing which reproduces the current neutrino masses…

高能物理 - 唯象学 · 物理学 2022-08-19 Victoria Puyam , S. Robertson Singh , N. Nimai Singh

Motivated by the flavored Peccei-Quinn symmetry for unifying the flavor physics and string theory, we construct an explicit model by introducing a $U(1)$ symmetry such that the $U(1)_X$-$[gravity]^2$ anomaly-free condition together with the…

高能物理 - 唯象学 · 物理学 2017-07-26 Y. H. Ahn

Sequestering is a promising mechanism in 4D string models to reconcile high-scale inflation with low-energy supersymmetry. In this scenario the MSSM lives on branes at singularities and it is sequestered from the sources of supersymmetry…

高能物理 - 理论 · 物理学 2023-09-15 Michele Cicoli , Alessandro Cotellucci , Hajime Otsuka

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

We study the implications of a large nu_mu - nu_tau mixing angle on flavour changing transitions of quarks and leptons in supersymmetric extensions of the standard model. Two patterns of supersymmetry breaking are considered, models with…

高能物理 - 唯象学 · 物理学 2014-11-17 Wilfried Buchmuller , David Delepine , Laksana Tri Handoko

Neutrino flavor instabilities appear to be omnipresent in dense astrophysical environments, thus presenting a challenge to large-scale simulations of core-collapse supernovae and neutron star mergers (NSMs). Subgrid models offer a path…

高能天体物理现象 · 物理学 2025-05-27 Sherwood Richers , Julien Froustey , Somdutta Ghosh , Francois Foucart , Javier Gomez

This paper examines neutrino flavor evolution outside a supernova neutrinosphere using a one-dimensional model that retains the non-linear nature of neutrino-neutrino interactions as well as some aspects of the full geometry. In some…

高能天体物理现象 · 物理学 2015-06-26 B. D. Keister

We construct models of leptons based on $S_4$ family symmetry combined with a generalised CP symmetry $H_{CP}$. We show how the flavon potential can spontaneously break the symmetry $S_4 \rtimes H_{CP}$ down to $Z_2 \times H^{\nu}_{CP}$ in…

高能物理 - 唯象学 · 物理学 2015-06-15 Gui-Jun Ding , Stephen F. King , Christoph Luhn , Alexander J. Stuart

I suggest a new particle model to integrate the fermion flavor, the TeV scale Leptogenesis and cold dark matter. The model has a local gauge symmetry $U(1)_{B-L}$ at the TeV scale and a flavor family symmetry SO(3), in addition, it also…

高能物理 - 唯象学 · 物理学 2013-02-27 Wei-Min Yang

We study a modified version of the Standard Model that includes a scalar doublet and two right-handed neutrinos, forming the neutrinophillic two higgs doublet ($\nu\text{2HDM}$) framework. For $v_2 << v_1$, this model operates at a TeV…

高能物理 - 唯象学 · 物理学 2025-05-30 Abhishek , V. Suryanarayana Mummidi

We investigate the maximal approximate flavor symmetry in the framework of generic minimal supersymmetric standard model. We consider the low energy effective theory of the flavor physics with all the possible operators included.…

高能物理 - 唯象学 · 物理学 2007-05-23 Zhijian Tao
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