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相关论文: Neutrino masses from operator mixing

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The recent observational data supports the deviation from Tri-bimaximal (TBM) mixings. Different neutrino mass models suggest the interdependency among the observational parameters involving the mixing angles. On phenomenological ground we…

高能物理 - 唯象学 · 物理学 2015-06-11 Subhankar Roy , N. Nimai Singh

We study the generation of neutrino masses and mixing in supersymmetric R-parity violating models containing two pairs of Higgs doublets. In these models, new RPV terms $\hat H_{D_1} \hat H_{D_2} \hat E$ arise in the superpotential, as well…

高能物理 - 唯象学 · 物理学 2015-06-18 Yuval Grossman , Clara Peset

We analyze the structure of quark and lepton mass matrices under the hypothesis that they are determined from a minimum principle applied to a generic potential invariant under the $\left[SU(3)\right]^5\otimes \mathcal O(3)$ flavor…

高能物理 - 唯象学 · 物理学 2015-06-16 R. Alonso , M. B. Gavela , G. Isidori , L. Maiani

In an extension of the minimal supersymmetric standard model (popularly known as the $\mu\nu$SSM), three right handed neutrino superfields are introduced to solve the $\mu$-problem and to accommodate the non-vanishing neutrino masses and…

高能物理 - 唯象学 · 物理学 2014-11-20 Pradipta Ghosh , Paramita Dey , Biswarup Mukhopadhyaya , Sourov Roy

Conventionally, neutrino masses in a supersymmetric theory arise from non-renormalizable lepton-number (L)-violating operators in the superpotential. The alternative possibility of having such operators in the Kahler potential as the…

高能物理 - 唯象学 · 物理学 2009-11-07 J. A. Casas , J. R. Espinosa , I. Navarro

Current solar and atmospheric neutrino oscillation data seem to favor a bimaximal pattern for neutrino mixings where the matrix elements U_{e2} and U_{\mu 3} are of order one, while U_{e3} is much smaller. We show that such a pattern can be…

高能物理 - 唯象学 · 物理学 2011-05-12 K. S. Babu , S. M. Barr

We construct a realistic model based on SUSY SO(10) with U(2) flavor symmetry. A set of symmetric mass textures give rise to very good predictions; 15 masses and 6 mixing angles are predicted by 11 parameters. Both the vacuum oscillation…

高能物理 - 唯象学 · 物理学 2007-05-23 Mu-Chun Chen , K. T. Mahanthappa

A $Z_{2L}\times Z_{2R}$ generation symmetry in the neutrino sector predicts the atmospheric neutrino mixing to be maximal, and the MNS matrix element $U_{e3}$ to be zero, consistent with observations. Solar neutrino mixing may be maximal…

高能物理 - 唯象学 · 物理学 2007-05-23 C. S. Lam

Considering the scheme with mixing of three neutrinos and a mass hierarchy that can accommodate the results of solar and atmospheric neutrino experiments, it is shown that the results of solar neutrino experiments imply a lower bound for…

高能物理 - 唯象学 · 物理学 2009-10-31 C. Giunti

We present an $A4$-based model where neutrino masses arise from a combination of see-saw mechanisms. The model is motivated by several small mixing and mass parameters indicated by the data. These are $\theta_{13}$, the solar mass…

高能物理 - 唯象学 · 物理学 2016-03-04 Soumita Pramanick , Amitava Raychaudhuri

We discuss consequences of assuming that the (Majorana) neutrino mass matrix $M_\nu$ and the charged lepton mass matrix $M_l$ satisfy, $S_\nu^T M_\nu S_\nu=-M_\nu~,T_l^\dagger M_lM_l^\dagger T_l=M_lM_l^\dagger$ with respect to some discrete…

高能物理 - 唯象学 · 物理学 2016-08-31 Anjan S Joshipura , Newton Nath

The observed neutrino mixing, having a near maximal atmospheric neutrino mixing angle and a large solar mixing angle, is close to tri-bi-maximal. We argue that this structure suggests a family symmetric origin in which the magnitude of the…

高能物理 - 唯象学 · 物理学 2008-11-26 I. de Medeiros Varzielas , S. F. King , G. G. Ross

In these two lectures I describe first the theory of neutrino mass and then discuss the implications of recent data (including 708--day data Super--Kamiokande data) which strongly indicate the need for neutrino conversions to account for…

高能物理 - 唯象学 · 物理学 2007-05-23 J. W. F. Valle

We investigate how the bi-large mixing required by the recent neutrino data can be accommodated in the supersymmetric standard model allowing bilinear R-parity violation and non-universal soft terms. In this scheme, the tree-level…

高能物理 - 唯象学 · 物理学 2010-04-05 E. J Chun , D. -W. Jung , J. D Park

Based on existing data, we argue for a peculiar structure of the neutrino mass matrix, that has a block of relatively large elements--a dominant block. We analyze this ansatz and extract its predictions, assuming that the O(1) coefficients…

高能物理 - 唯象学 · 物理学 2007-05-23 Francesco Vissani

Models, where neutrino mass originates from physics at the TeV scale and which are potentially testable at the LHC, need additional suppression mechanisms to describe the smallness of neutrino masses. We consider models in which neutrino…

高能物理 - 唯象学 · 物理学 2013-07-17 Martin B. Krauss , Davide Meloni , Werner Porod , Walter Winter

If, as suggested by the SuperKamiokande results, the mu neutrino and tau neutrino are maximally and ``rapidly'' mixed, this alone determines the mapping from current to mass eigenstates up to one rotation angle (theta) mixing the electron…

高能物理 - 唯象学 · 物理学 2009-10-31 Anthony J. Baltz , Alfred Scharff Goldhaber , Maurice Goldhaber

We evaluate the predictive power of the neutrino mass matrices arising from seesaw mechanism with heavy Majorana mass matrices subject to texture zero and satisfy a cyclic permutation invariant form to the solar neutrino mixing phenomena.…

高能物理 - 唯象学 · 物理学 2010-09-21 Asan Damanik , Mirza Satriawan , Pramudita Anggraita , Arief Hermanto , Muslim

We review some fundamental aspects of the theory of neutrino masses and mixing. The results of neutrino oscillation experiments are interpreted as evidence of three-neutrino mixing. Implications for the mixing parameters and the neutrino…

高能物理 - 唯象学 · 物理学 2008-11-26 Carlo Giunti

We suggest an approach to explain the observed pattern of the neutrino masses and mixing which employs the weakly broken quark-lepton symmetry and does not require introduction of an ad hoc symmetry of the neutrino sector. The mass matrices…

高能物理 - 唯象学 · 物理学 2009-11-10 I. Dorsner , A. Yu. Smirnov