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相关论文: Predictive Model of Inverted Neutrino Mass Hierarc…

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The comprehensive analyses are presented in the model with the inverted mass hierarchy for neutrinos, which follows from a geometrical structure of a (1+5) dimensional space-time where two extra dimensions are compactified on the T^2/Z_3…

高能物理 - 唯象学 · 物理学 2008-11-26 Mizue Honda , Morimitsu Tanimoto

The recent measurement of a non-zero neutrino mixing angle $\theta_{13}$ requires a modification of the tri-bimaximal mixing pattern that predicts a zero value for it. We propose a new neutrino mixing pattern based on a spontaneously-broken…

高能物理 - 唯象学 · 物理学 2013-05-30 Y. H. Ahn , Seungwon Baek , Paolo Gondolo

Best-fit values of recent global analyzes of neutrino data imply large solar neutrino mixing, vanishing U_{e3} and a non-maximal atmospheric neutrino mixing angle theta_{23}. We show that these values emerge naturally by the hypothesis of…

高能物理 - 唯象学 · 物理学 2008-11-26 A. Blum , R. N. Mohapatra , W. Rodejohann

We propose a particularly economical neutrino mass model, in which there are only two right-handed Majorana neutrinos of ${\cal O}(1)$ TeV and their masses are highly degenerate. Its novel Yukawa-coupling texture together with the seesaw…

高能物理 - 唯象学 · 物理学 2008-11-26 Zhi-zhong Xing , Shun Zhou

Motivated by effective low energy models of string origin, we discuss the neutrino masses and mixing within the context of the Minimal Supersymmetric Standard Model supplemented by a U(1) anomalous family symmetry and additional Higgs…

高能物理 - 唯象学 · 物理学 2009-11-11 G. K. Leontaris , A. Psallidas , N. D. Vlachos

A non-supersymmetric inverse seesaw model of neutrino mass based on the $A^{\prime}_5$ modular symmetry is presented. This framework provides a combined explanation for neutrino masses, mixing, and the cosmic baryon asymmetry through…

高能物理 - 唯象学 · 物理学 2026-03-20 Xianshuo Zhang , Yakefu Reyimuaji

We propose a minimal inverse seesaw model with $S_4$ symmetry for the Majorana neutrinos with only one real ($m_0$)-and two complex ($\alpha, \beta$) parameters in neutrino sector which gives reasonable predictions for the neutrino…

高能物理 - 唯象学 · 物理学 2025-11-25 V. V. Vien , Mayengbam Kishan Singh

Combining the KSVZ axion model and the type-I seesaw mechanism, we construct a minimal flavored axion model that can affect the neutrino mass matrix. This minimal model requires a flavor dependent PQ charge assignment and two additional…

高能物理 - 唯象学 · 物理学 2025-07-01 Zhen-Yu Lei , Jian-Wei Cui

We have studied the scenario of baryogenesis via leptogenesis in an $A_4$ flavor symmetric framework considering type I seesaw as the origin of neutrino mass. Because of the presence of the fifth generation right handed neutrino the model…

高能物理 - 唯象学 · 物理学 2018-03-23 Ananya Mukherjee , Mrinal Kumar Das , Jayanta Kumar Sarma

We study models of neutrino masses which naturally give rise to an inverted mass hierarchy and bi-maximal mixing. The models are based on the see-saw mechanism with three right-handed neutrinos, which generates a single mass term of the…

高能物理 - 唯象学 · 物理学 2009-10-31 S. F. King , N. Nimai Singh

We present a low-scale type-I seesaw scenario with discrete flavor and CP symmetries. This scenario not only explains the measured values of the lepton mixing angles, but also makes predictions for leptonic CP violation, and connects the…

高能物理 - 唯象学 · 物理学 2023-01-03 Garv Chauhan , P. S. Bhupal Dev

An attempt is made to explore the possibility for deviations of solar mixing angle ($\theta_{12}$) from tri-bimaximal mixings, without sacrificing the predictions of maximal atmospheric mixing angle ($\theta_{23}=\pi/4$) and zero reactor…

高能物理 - 唯象学 · 物理学 2008-11-26 N. Nimai Singh , Monisa Rajkhowa , Abhijit Borah

We present successful lepton mass matrices with an inverted mass hierarchy for neutrinos, which follow from a geometrical structure of a (1+5) dimensional space-time where two extra dimensions are compactified on the T^2/Z_3 orbifold. A 5^*…

高能物理 - 唯象学 · 物理学 2009-11-11 M. Tanimoto , T. Yanagida

We discuss a class of models of neutrino masses and mixings with inverse hierarchy based on a broken U(1)_F flavour symmetry with charge L_e-L_\mu-L_\tau for lepton doublets and arbitrary right-handed charges. The symmetry breaking sector…

高能物理 - 唯象学 · 物理学 2010-02-03 Guido Altarelli , Roberto Franceschini

In the present work, the inverted hierarchical neutrino mass model which is characterised by opposite CP parity in the first two mass eigenvalues $(m_1,-m_2,m_3)$, is studied in order to lower the predicted value of solar mixing angle…

高能物理 - 唯象学 · 物理学 2008-11-26 N. Nimai Singh , Monisa Rajkhowa , Abhijit Borah

Starting from the symmetry of lepton flavor democracy, we propose and discuss a simple pattern for the mass generation and flavor mixing of the charged leptons and neutrinos. The three neutrino masses are nearly degenerate, and the flavor…

高能物理 - 唯象学 · 物理学 2009-10-28 H. Fritzsch , Z. Z Xing

The presently available information on neutrino oscillations can be used to tightly constrain the light neutrino mass matrix $m_\n$ under the assumption that the three known neutrinos provide explanation of the solar and atmospheric…

高能物理 - 唯象学 · 物理学 2007-05-23 Anjan S. Joshipura , Emmanuel A. Paschos

We present a model for lepton masses and mixing angles using the deconstruction setup, based on a non-Abelian flavor symmetry which is a split extension of the Klein group. The symmetries enforce an approximately maximal atmospheric mixing…

高能物理 - 唯象学 · 物理学 2007-05-23 Gerhart Seidl

We present a model based on an O(3) flavor symmetry and a minimal extension of the scalar sector to induce hierarchical breaking, O(3) -> O(2) -> SO(2) -> nothing. The model naturally accounts for all the known lepton parameters and yields…

高能物理 - 唯象学 · 物理学 2009-10-31 Gilad Perez

The current work involves augmenting the $\Delta(54)$ discrete flavor model by incorporating two Standard Model Higgs particles into the Inverse Seesaw mechanism. We introduced Weyl fermions and Vector like fermions, which are gauge…

高能物理 - 唯象学 · 物理学 2024-03-01 Hrishi Bora , Ng. K. Francis , Bikash Thapa , Shawan Kumar Jha
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