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相关论文: Twisted Family Structure and Neutrino Large Mixing

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We show that the neutrino masses with large mixing between \nu_\mu and \nu_\tau are naturally reproduced in a supersymmetric E_6 grand unification model with an anomalous U(1)_X symmetry. We propose a simple scenario which incorporates a…

高能物理 - 唯象学 · 物理学 2009-10-31 Masako Bando , Taichiro Kugo

A novel relation is found which gives the 2-3 lepton mixing angle in terms of quark masses and CKM mixing: \tan\theta_{\mu\tau}=(m_b/m_s)V_{cb}. This relation, which is remarkably in good agreement with the quark data and the large lepton…

高能物理 - 唯象学 · 物理学 2009-10-31 Masako Bando , Taichiro Kugo , Koichi Yoshioka

Mass matrix of quarks is studied in the Supersymmetric $E_6$ Grand Unified Theory (GUT). The fundamental representation $\textbf{27}$ in $E_6$ which corresponds to one generation contains two sets of $\textbf{5}^{*}$'s in SU(5), so that…

高能物理 - 唯象学 · 物理学 2007-05-23 Midori Obara , Gi-Chol Cho , Makiko Nagashima , Akio Sugamoto

We show that the large mixing between $\nu_\mu$ and $\nu_\tau$ observed by the SuperKamiokande collaboration is a quite natural prediction in a large class of seesaw models. This large mixing is basically due to the unparallel family…

高能物理 - 唯象学 · 物理学 2009-10-31 J. Sato , T. Yanagida

We study a coset-space unification model for families based on $E_7/SU(5) \times U(1)^3$. We find that qualitative structure of quark and lepton mass matrices in this model describes very well the observation. We stress, in particular, that…

高能物理 - 唯象学 · 物理学 2016-09-06 J. Sato , T. Yanagida

The observed quark hierarchies suggest a simple family symmetry. Generalized to leptons through grand-unified quantum numbers, it produces a neutrino mixing matrix with order-one \nu_{\mu} - \nu_{\tau} mixing, and order-\lambda^3 \nu_e -…

高能物理 - 唯象学 · 物理学 2009-10-31 John K. Elwood , Nikolaos Irges , Pierre Ramond

The recent data describing the evidence for neutrino oscillations by Super Kamiokande implies that two neutrinos are very strongly mixed. We ask the question: can approximate maximal neutrino mixing be natural in unified (GUT or string)…

高能物理 - 唯象学 · 物理学 2009-10-31 B. C. Allanach

We discussed neutrino masses and mixings in SUSY SO(10) model where quarks and leptons have Yukawa couplings to at least two 10 and one $\bar{126}$ Higgs scalars. In this model, the Dirac and the right-handed Majorana mass terms are…

高能物理 - 唯象学 · 物理学 2008-11-26 Kin-ya Oda , Eiichi Takasugi , Minoru Tanaka , Masaki Yoshimura

An alternative supersymmetric SO(10) grand unification model with lopsided fermion mass matrices is introduced. It generates a large solar-neutrino-mixing angle through the neutrinos' Dirac mass matrix constrained by the SO(10) group…

高能物理 - 唯象学 · 物理学 2009-11-11 Xiangdong Ji , Yingchuan Li , R. N. Mohapatra

We investigate the SO(10) grand unified model with generation flipping. The model contains one extra matter multiplet $\psi(10)$ and it mixes with the usual matter multiplets $\psi_i(16)$ when the SO(10) is broken down to SU(5). We find the…

高能物理 - 唯象学 · 物理学 2009-09-29 Yasunori Nomura , Takashi Sugimoto

The generation of the fermion mass hierarchy in the standard model of particle physics is a long-standing puzzle. The recent discoveries from neutrino physics suggests that the mixing in the lepton sector is large compared to the quark…

高能物理 - 唯象学 · 物理学 2008-11-26 David McKeen , Jonathan L. Rosner , Arun M. Thalapillil

Assuming grand unified theory (GUT) and supersymmetry, we propose a simple model which can consistently accommodate the masses and mixings for quarks and leptons. The grand unified group is SO(10), and $\bf 10$, $\bf 120$, and $\bar {\bf…

高能物理 - 唯象学 · 物理学 2009-11-10 Noriyuki Oshimo

Near maximal neutrino mixing needed to understand atmospheric neutrino data can be interpreted to be a consequence of an interchange symmetry between the muon and tau neutrinos in the neutrino mass matrix in the flavor basis. This idea can…

高能物理 - 唯象学 · 物理学 2009-11-11 R. N. Mohapatra , S. Nasri , Hai-Bo Yu

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

Within the framework of grand unified theories, we make full analysis of symmetric texture to see if such texture can reproduce large neutrino mixings, which have recently been confirmed by the observed solar and atmospheric neutrino…

高能物理 - 唯象学 · 物理学 2009-11-10 Masako Bando , Midori Obara

Seesaw mechanism appears to be the simplest and most appealing way to understand small neutrino masses observed in recent experiments. It introduces three right handed neutrinos with heavy masses to the standard model, with at least one…

高能物理 - 唯象学 · 物理学 2014-11-18 R. N. Mohapatra

We describe a supersymmetric Grand Unified Theory based on the gauge group $\SU(5)^3$, or $\SO(10)^3$, invariant under the interchange of any~SU(5), or~SO(10), with each family multiplet transforming non trivially under one different…

高能物理 - 唯象学 · 物理学 2009-10-09 Riccardo Barbieri , Gia Dvali , Alessandro Strumia

Using the family symmetry, in the neutrino mass matrix we remove the Yukawa coupling (arising in the Dirac type mass between the heavy neutrinos and light lepton doublets) dependence in the double seesaw mechanism so that it is directly…

高能物理 - 唯象学 · 物理学 2009-11-11 Jihn E. Kim , Jong-Chul Park

We consider the problem of neutrino masses and mixing angles in a supersymmetric model based on the gauge group SU(4)$\otimes$SU(2)$_L\otimes$SU(2)$_R$ broken at the scale $M_X\approx 10^{16}$ GeV. We extend a previous operator analysis of…

高能物理 - 唯象学 · 物理学 2009-10-28 B. C. Allanach , S. F. King

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
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