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相关论文: The Simplest Neutrino Mass Matrix

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We consider the simplest model which solves the solar and atmospheric neutrino puzzles, in the sense that it contains the smallest amount of beyond the Standard Model ingredients. The solar neutrino data is accounted for by Planck-mass…

高能物理 - 唯象学 · 物理学 2009-09-17 Andre de Gouvea , J. W. F. Valle

In spite of enormous experimental progress in determination of the neutrino parameters, theory of neutrino mass and mixing is still on the cross-roads. Guidelines could be (i) the connection between zero neutrino charges (and therefore a…

高能物理 - 唯象学 · 物理学 2022-03-02 Alexei Yu. Smirnov

With the recent experimental advance in our precise knowledge of the neutrino oscillation parameters, the correct form of the 3 X 3 neutrino mass matrix is now approximately known. I discuss how this may be obtained from symmetry…

高能物理 - 唯象学 · 物理学 2008-11-26 Ernest Ma

A universal seesaw mass matrix model, which gives successful description of quark mass matrix in terms of lepton masses, yields three "sterile" neutrinos \nu^s_{i}, which compose pseudo-Dirac neutrinos \nu_{i\pm}^{ps}\simeq (\nu_{i} \pm…

高能物理 - 唯象学 · 物理学 2009-10-31 Yoshio Koide , Hideo Fusaoka

Assuming lepton number conservation, hermiticity of the neutrino mass matrix and $\nu_{\mu} - \nu_{\tau}$ exchange symmetry, we show that we can determine the neutrino mass matrix completely from the existing data. Comparing with the…

高能物理 - 唯象学 · 物理学 2014-05-26 Shreyashi Chakdar , Kirtiman Ghosh , S. Nandi

In the context of a minimal extension of the Standard Model with three extra heavy right-handed neutrinos, we propose a model for neutrino masses and mixing based on the hipothesis of a complete alignment of the lepton mass matrices in…

高能物理 - 唯象学 · 物理学 2009-10-31 F. R. Joaquim

When the neutrino mass eigenstate $\nu_2$ is trimaximally mixed, the mixing matrix is called trimaximal. The middle column of trimaximal mixing matrix is identical to tri-bimaximal mixing and the other two columns are subject to unitarity…

高能物理 - 唯象学 · 物理学 2013-08-02 Sanjeev Kumar

Neutrino oscillations are one of the most studied and successful phenomena since the establishment of the solar neutrino problem in late 1960's. In this work we discuss the exact expressions for the probability P_{\alpha\beta} in a constant…

高能物理 - 唯象学 · 物理学 2016-11-23 L. J. Flores , O. G. Miranda

The correct quark and charged lepton mass matrices along with a nearly correct CKM matrix may be naturally accommodated in a Pati-Salam model constructed from intersecting D6 branes on a $T^6/(\Z_2 \times \Z_2)$ orientifold. Furthermore,…

高能物理 - 唯象学 · 物理学 2020-01-01 Jordan Gemmill , Evan Howington , Van E. Mayes

We study in detail the sensitivity of neutrino oscillation probabilities to the fundamental neutrino parameters and their possible determination through experiments. The first part of the paper is devoted to the broad theme of isolating…

高能物理 - 唯象学 · 物理学 2009-11-11 D. Indumathi , M. V. N. Murthy , G. Rajasekaran , Nita Sinha

Inspired by the recent T2K indication of a relatively large theta_{13}, we provide a systematic study of some general modifications to three mostly discussed neutrino mixing patterns, i.e., tri-bimaximal, bimaximal and democratic mixing…

高能物理 - 唯象学 · 物理学 2011-07-06 Wei Chao , Ya-juan Zheng

We analyze the neutrino mass matrix entries and their correlations in a probabilistic fashion, constructing probability distribution functions using the latest results from neutrino oscillation fits. Two cases are considered: the standard…

高能物理 - 唯象学 · 物理学 2015-06-12 E. Bertuzzo , P. A. N. Machado , R. Zukanovich Funchal

We investigate the quantum effects for the democratic-type neutrino mass matrix given at the right-handed neutrino mass scale $m_R$ in order to see (i) whether $\theta_{23}=-\pi/4$ predicted by the model is stable to explain the atmospheric…

高能物理 - 唯象学 · 物理学 2009-10-31 Takahiro Miura , Eiichi Takasugi , Masaki Yoshimura

With the latest astronomical data including Cosmic Microwave Background (WMAP three year, CBI, ACBAR, VSA), Type Ia Supernova ("gold sample"), Galaxy Clustering (SDSS 3-D matter power, Lyman-$\alpha$ forest and Baryon Acoustic Oscillating…

天体物理学 · 物理学 2010-10-27 Gong-Bo Zhao , Jun-Qing Xia , Xinmin Zhang

We present a simple modification of the Altarelli-Feruglio $A_4$ flavor symmetry model using a minimal number of parameters congruous with the symmetries of the original theory. The resulting model is consistent with all presently known…

高能物理 - 唯象学 · 物理学 2020-08-05 Minjie Lei , James D. Wells

Current neutrino data are consistent with the so-called tribimaximal mixing scenario, which predicts \sin^2 \theta_{12}=1/3, zero U_{e3} and maximal \theta_{23}. This implies a special form of the neutrino mass matrix. Introducing small…

高能物理 - 唯象学 · 物理学 2014-11-18 F. Plentinger , W. Rodejohann

The present manuscript studies a recently proposed new neutrino mixing scheme with a neutrino mass selection rule, $m_{\nu}^{13} + m_{\nu}^{22} + m_{\nu}^{31} = 0$, among a neutrino mass matrix elements. The neutrino mass matrix texture is…

高能物理 - 唯象学 · 物理学 2026-01-05 Takaaki Nomura , Oleg Popov

We discuss neutrino sector in models with two Higgs doublet and one singlet scalar fields under local $U(1)_{L_\alpha- L_\beta}$ symmetry. A neutrino mass matrix is formulated for these models where the matrix is generated via type-I seesaw…

高能物理 - 唯象学 · 物理学 2025-01-28 Yuanchao Lou , Takaaki Nomura

Global fits to all data of candidates for neutrino oscillations are presented in the framework of a three-flavor model. The analysis excludes mass regions where the MSW effect is important for the solar neutrino problem. The best fit gives…

高能物理 - 唯象学 · 物理学 2016-08-25 Tommy Ohlsson , Hakan Snellman

We endeavor to constrain the neutrino mass matrix on the phenomenological ground and procure model-independent textures by emphasizing on the simple linear relationships among the mass matrix elements. These simple textures predict the two…

高能物理 - 唯象学 · 物理学 2024-01-29 Pralay Chakraborty , Manash Dey , Subhankar Roy
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