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相关论文: Golden Ratio Prediction for Solar Neutrino Mixing

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We present a simple texture that predicts the cotangent of the solar neutrino mixing angle to be equal to the golden ratio. This prediction is 1.4 standard deviations below the present best-fit value and final SNO and KamLAND data could…

高能物理 - 唯象学 · 物理学 2008-11-26 Yuji Kajiyama , Martti Raidal , Alessandro Strumia

We investigate the possibility of using icosahedral symmetry as a family symmetry group in the lepton sector. The rotational icosahedral group, which is isomorphic to A5, the alternating group of five elements, provides a natural context in…

高能物理 - 唯象学 · 物理学 2010-04-23 Lisa L. Everett , Alexander J. Stuart

We formulate a consistent model predicting, in the leading order approximation, maximal atmospheric mixing angle, vanishing reactor angle and tan {\theta}_12 = 1/{\phi} where {\phi} is the Golden Ratio. The model is based on the flavour…

高能物理 - 唯象学 · 物理学 2015-03-17 Ferruccio Feruglio , Alessio Paris

We furnish a supersymmetric extension of the Standard Model with a flavour discrete symmetry $A_5$ under which the lepton fields transform as an irreducible triplet. Additional (`flavon') superfields are used to break $A_5$ into a…

高能物理 - 唯象学 · 物理学 2015-06-18 I. de Medeiros Varzielas , L. Lavoura

Flavor symmetry ($T^{'} \times Z_2$) where $T^{'}$ is the binary tetrahedral group predicts for neutrino mixing angles $\theta_{13} = \sqrt{2} (\frac{\pi}{4} - \theta_{23})$ and, with one phenomenological input, provides upper and lower…

高能物理 - 唯象学 · 物理学 2010-04-21 David A. Eby , Paul H. Frampton , Shinya Matsuzaki

We propose a new parametrization for the quark and lepton mixing matrices: the two 12-mixing angles (the Cabibbo angle and the angle responsible for solar neutrino oscillations) are at zeroth order pi/12 and pi/5, respectively. The…

高能物理 - 唯象学 · 物理学 2010-04-21 Werner Rodejohann

The trimaximal mixing scheme is one of the widely studied neutrino mixing schemes. However, the predicted solar neutrino mixing angle $\theta_{12}$ and the reactor neutrino mixing angle $\theta_{13}$ cannot simultaneously realize their…

高能物理 - 唯象学 · 物理学 2023-11-27 Yulin Chen , Yuta Hyodo , Teruyuki Kitabayashi

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 provide a systematic and thorough exploration of lepton flavor models in which the solar mixing angle is related to the golden ratio. For scenarios in which the solar mixing angle is given by the inverse cotangent of the golden ratio, we…

高能物理 - 唯象学 · 物理学 2012-01-10 Gui-Jun Ding , Lisa L. Everett , Alexander J. Stuart

In drawing on an analogy with the flavor mixing observed in the quark sector we discuss a pattern of large flavor mixing angles in the lepton sector. Simple arguments based on a democratic symmetry and its violation in the lepton sector…

高能物理 - 唯象学 · 物理学 2007-05-23 Harald Fritzsch , Zhi-Zhong Xing

We show how the neutrino mixing angles and oscillation phase can be predicted from tri-bimaximal neutrino mixing, corrected by charged lepton mixing angles which are related to quark mixing angles via quark-lepton unification. The…

高能物理 - 唯象学 · 物理学 2009-11-11 S. F. King

We discuss the neutrino mixing, using the texture 0 mass matrices, which work very well for the quarks. The solar mixing angle is directly linked to the mass ratio of the first two neutrinos. The neutrino masses are hierarchical, but the…

高能物理 - 唯象学 · 物理学 2008-11-26 H. Fritzsch

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

In a new application of the discrete non-Abelian symmetry A_4 using the canonical seesaw mechanism, a three-parameter form of the neutrino mass matrix is derived. It predicts the following mixing angles for neutrino oscillations:…

高能物理 - 唯象学 · 物理学 2009-11-11 Ernest Ma

Neutrino mixing matrix appears to be close to bimaximal mixing, but for the solar mixing angle which is definitively smaller than forty five degrees. Whereas it seems quite easy to understand bimaximal mixing with the use of new global…

高能物理 - 唯象学 · 物理学 2008-11-26 J. C. Gómez-Izquierdo , A. Pérez-Lorenzana

The requirement of the mu-tau symmetry in the neutrino sector that yields the maximal atmospheric neutrino mixing is shown to yield either sin(\theta_{13})=0 (referred to as C1)) or sin(\theta_{12})=0 (referred to as C2)), where…

高能物理 - 唯象学 · 物理学 2009-11-11 Kenichi Fuki , Masaki Yasue

Small discrete family symmetries such as S4, A4 or A5 may lead to simple leading-order predictions for the neutrino mixing matrix such as the bimaximal, tribimaximal or golden ratio mixing patterns, which may be brought into agreement with…

高能物理 - 唯象学 · 物理学 2015-06-23 Peter Ballett , Stephen F. King , Christoph Luhn , Silvia Pascoli , Michael A. Schmidt

Flavour symmetries appropriate for describing a neutrino spectrum with degenerate solar pair and a third massive or massless neutrino are discussed. We demand that the required residual symmetries of the leptonic mass matrices be subgroups…

高能物理 - 唯象学 · 物理学 2014-08-27 Anjan S. Joshipura , Ketan M. Patel

When solar neutrino and KamLAND data are analyzed separately one finds that, even though allowed regions of neutrino parameters overlap, the values of $\delta m^2$ and the mixing angle $\theta_{12}$ at the $\chi^2$ minima are different. We…

高能物理 - 唯象学 · 物理学 2008-11-26 A. B. Balantekin , D. Yilmaz

Using group theory of mixing to examine all finite subgroups of SU(3) with an order less than 512, we found recently that only the group $\Delta(150)$ can give rise to a correct reactor angle $\th_{13}$ of neutrino mixing without any free…

高能物理 - 唯象学 · 物理学 2015-06-12 C. S. Lam
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