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相关论文: Nonzero theta_13 signals nonmaximal atmospheric ne…

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We suggest a minimal extension of the simplest A4 flavour model that can induce a nonzero theta13 value, as required by recent neutrino oscillation data from reactors and accelerators. The predicted correlation between the atmospheric…

高能物理 - 唯象学 · 物理学 2013-08-09 S. Morisi , D. V. Forero , J. C. Romao , J. W. F. Valle

We show that seesaw models based on flavor symmetries (such as A_4 and Z_7 X Z_3) which produce exact tribimaximal neutrino mixing, also imply a vanishing leptogenesis asymmetry. We show that higher order symmetry breaking corrections in…

高能物理 - 唯象学 · 物理学 2010-05-27 Elizabeth E. Jenkins , Aneesh V. Manohar

In the original 2004 paper which first derived tribimaximal mixing in the context of A(4), i.e. the non-Abelian finite symmetry group of the tetrahedron (Plato's fire), as its simplest application, it was also pointed out how theta(13)…

高能物理 - 唯象学 · 物理学 2011-12-26 Ernest Ma , Daniel Wegman

One of the most robust relationships predicted by binary tetrahedral ($T^{'}$) flavor symmetry relates the reactor neutrino angle $\theta_{13}$ to the atmospheric neutrino angle $\theta_{23}$, independently of $\theta_{12}$. It has the form…

高能物理 - 唯象学 · 物理学 2017-07-06 Paul H. Frampton

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 present a model of neutrino mixing based on the flavour group $\Delta(27)$ in order to account for the observation of a non-zero reactor mixing angle ($\theta_{13}$). The model provides a common flavour structure for the charged-lepton…

高能物理 - 唯象学 · 物理学 2014-06-10 P. F. Harrison , R. Krishnan , W. G. Scott

Motivated by recent observations of non-zero $\theta_{13}$ from the Daya Bay and RENO experiments, we propose a renormalizable neutrino model with $A_4$ discrete symmetry accounting for deviations from the tri-bimaximal mixing pattern of…

高能物理 - 唯象学 · 物理学 2015-06-04 Y. H. Ahn , Sin Kyu Kang

The tetra-maximal neutrino mixing pattern predicts a relatively large reactor mixing angle theta_13 \approx 8.4^\circ, which is in good agreement with the latest best-fit value theta_13 = 9^\circ. However, its prediction for theta_12…

高能物理 - 唯象学 · 物理学 2015-05-28 He Zhang , Shun Zhou

The binary tetrahedral group ($T^{'}$) has provided the most successful flavour symmetry in understanding simultaneously the three mixing angles both for quarks in the CKM matrix and for neutrinos in the PMNS matrix. One prediction,…

高能物理 - 唯象学 · 物理学 2023-09-07 Claudio Corianò , Paul H. Frampton , Pietro Santorelli

We provide a short summary of three-flavour neutrino oscillation parameters as determined from a global fit to 2008 data, and we comment on possible hints in favour of a non-zero value of the mixing angle theta_{13} found in…

高能物理 - 唯象学 · 物理学 2010-02-17 Michele Maltoni , Thomas Schwetz

In study of muon neutrino disappearance at 810 km, the NOvA experiment finds flavor mixing of the atmospheric sector to deviate from maximal ($\sin^2\theta_{23} = 0.5$) by 2.6 $\sigma$. The result is in tension with the 295-km baseline…

高能物理 - 唯象学 · 物理学 2017-06-07 Joao A. B. Coelho , W. Anthony Mann , Saqib S. Bashar

A simple three-flavor neutrino-oscillation model is discussed which has both nonzero mass differences and timelike Fermi-point splittings, together with a combined bi-maximal and trimaximal mixing pattern. One possible consequence would be…

高能物理 - 唯象学 · 物理学 2014-11-18 Frans R. Klinkhamer

We discuss how \theta_{13} \neq 0 is accommodated in a recently proposed renormalizable model of neutrino mixing using the non-Abelian discrete symmetry T_7 in the context of a supersymmetric extension of the Standard Model with gauged…

高能物理 - 唯象学 · 物理学 2013-05-29 Qing-Hong Cao , Shaaban Khalil , Ernest Ma , Hiroshi Okada

An extension of the neutrino sector with two right handed singlet neutrinos responsible for Dirac neutrino masses is discussed. We show that this setup with flavor symmetry can give large solar and atmospheric neutrino mixings and…

高能物理 - 唯象学 · 物理学 2008-11-26 S. Nandi , Zurab Tavartkiladze

For a neutrino mass matrix whose texture has an approximate flavor symmetry and where one has near degenerate neutrino mass, it is shown that the tribimaximal values for atmospheric angle $\sin^{2}{\theta_{23}}=1/2$ and solar angle…

高能物理 - 唯象学 · 物理学 2015-05-30 Riazuddin

In this addendum to arXiv:1103.0734 we consider the recent results from long-baseline $\nu_\mu\to\nu_e$ searches at the T2K and MINOS experiments and investigate their implications for the mixing angle $\theta_{13}$ and the leptonic Dirac…

高能物理 - 唯象学 · 物理学 2015-05-30 Thomas Schwetz , Mariam Tortola , J. W. F. Valle

The neutrino mixing angle theta(13) is at the focus of current neutrino research. From a global analysis of the available oscillation data in a 3-neutrino framework, we previously reported [Phys. Rev. Lett. 101, 141801 (2008)] hints in…

高能物理 - 唯象学 · 物理学 2013-05-29 G. L. Fogli , E. Lisi , A. Marrone , A. Palazzo , A. M. Rotunno

We present the lepton flavor model with $\Delta (54)$, which appears typically in heterotic string models on the $T^2/Z_3$ orbifold. Our model reproduces the tri-bimaximal mixing in the parameter region around degenerate neutrino masses or…

高能物理 - 唯象学 · 物理学 2010-04-30 Hajime Ishimori , Tatsuo Kobayashi , Hiroshi Okada , Yusuke Shimizu , Morimitsu Tanimoto

Here we study the pattern of neutrino oscillations emerging from a previously proposed warped model construction incorporating $\Delta(27)$ flavor symmetry. In addition to a complete description of fermion masses, the model predicts the…

高能物理 - 唯象学 · 物理学 2017-06-07 Pedro Pasquini , S. C. Chuliá , J. W. F. Valle

By postulating the relation \theta_{23} \simeq 45^\circ + \eta\theta_{13}, we seek preferable correction terms to tri-bi-maximal mixing and discuss their origins. Global analyses of the neutrino oscillation parameters favor \eta=\pm…

高能物理 - 唯象学 · 物理学 2014-05-07 Takeshi Araki
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