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相关论文: Perturbing exactly tri-bimaximal neutrino mixings …

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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 recent measurement of the third lepton mixing angle, \theta_{13}, has shown that, although small compared to \theta_{12} and \theta_{23}, it is much larger than anticipated in schemes that generate Tri-Bi-Maximal (TBM) or Golden Ratio…

高能物理 - 唯象学 · 物理学 2015-06-15 L. J. Hall , G. G. Ross

We construct phenomenologically viable models of lepton masses and mixing based on modular $A_4$ invariance broken to residual symmetries $\mathbb{Z}^{T}_3$ or $\mathbb{Z}^{ST}_3$ and $\mathbb{Z}^S_2$ respectively in the charged lepton and…

高能物理 - 唯象学 · 物理学 2019-05-22 P. P. Novichkov , S. T. Petcov , M. Tanimoto

The present article is an endeavor to look into some fruitful frameworks based on "Bi-maximal" neutrino mixing, from a model independent stand. The possibilities involving the correction or attenuation of the original BM mixing matrix,…

高能物理 - 唯象学 · 物理学 2016-03-28 Subhankar Roy , N. Nimai Singh

We introduce a new texture for neutrino mixing named Tri-Permuting (TP) mixing matrix. This pattern is characterized by maximal solar and atmospheric angles and by a large reactor angle satisfying sin(theta_13)=1/3. The correct lepton…

高能物理 - 唯象学 · 物理学 2015-03-19 F. Bazzocchi

We investigate in a model-independent way to what extent one can perturb tri-bimaximal mixing in order to generate a sizable value of |U_{e3}|, while at the same time keeping solar neutrino mixing near its measured value, which is close to…

高能物理 - 唯象学 · 物理学 2009-09-30 Srubabati Goswami , Serguey Petcov , Shamayita Ray , Werner Rodejohann

The solar and baseline neutrino oscillation data suggest bimaximal neutrino mixing among the first two generations, and trimaximal mixing between all three neutrino flavors. It has been conjectured that this indicates the existence of an…

高能物理 - 唯象学 · 物理学 2011-07-26 G. K. Leontaris , N. D. Vlachos

The tri-bimaximal mixing matrix is most likely the leading order term in the description of leptonic mixing. We derive deviations from tri-bimaximal mixing(TBM) due to corrections from the charged lepton sector. We assume a decoupled 2-3…

高能物理 - 唯象学 · 物理学 2008-09-17 Alakabha Datta

We propose a scheme, based on \Delta(27) flavor symmetry and supplemented by other discrete symmetries and inverse seesaw mechanism, where both the light neutrino masses and the deviation from tri-bimaximal mixing matrix can be linked to…

高能物理 - 唯象学 · 物理学 2016-01-27 M. Abbas , S. Khalil , A. Rashed , A. Sil

The neutrino mixing matrix U is in general of the form U=U_e^+ U_nu, where U_e arises from the diagonalization of charged leptons and U_nu is from the neutrino sector. We discuss the possibility that U_nu is nearly diagonal (in the…

高能物理 - 唯象学 · 物理学 2010-04-05 Guido Altarelli , Ferruccio Feruglio , Isabella Masina

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

Solar and atmospheric neutrino oscillations are consistent with a tribimaximal form of the mixing matrix $U$ of the lepton sector. Exact tribimaximal mixing leads to $\theta_{13}=0$. Recent results from the Daya Bay and RENO experiments…

高能物理 - 唯象学 · 物理学 2015-06-04 Biswajoy Brahmachari , Amitava Raychaudhuri

The recent results from T2K and MINOS experiments point towards a relatively large value of the reactor angle \theta_13 in the lepton sector. In this paper we show how a large \theta_13 can arise from the charged lepton sector alone in the…

高能物理 - 唯象学 · 物理学 2011-11-22 David Marzocca , Serguey T. Petcov , Andrea Romanino , Martin Spinrath

Current experimental data allow the zero value for one neutrino mass, either m_1 = 0 or m_3 = 0. This observation implies that a realistic neutrino mass texture can be established by starting from the limit (a) m_1 = m_2 = 0 and m_3 \neq 0…

高能物理 - 唯象学 · 物理学 2008-11-26 Aik Hui Chan , Harald Fritzsch , Shu Luo , Zhi-zhong Xing

We show that in a recently proposed $S_3$ model for tri-bimaximal mixing pattern for neutrinos, CP violating phases in neutrino mixings are directly responsible for lepton asymmetry $\epsilon_\ell$. In the exact tri-bimaximal limit,…

高能物理 - 唯象学 · 物理学 2008-11-26 R. N. Mohapatra , Hai-Bo Yu

In this paper, we consider a neutrino mass model based on $A_4$ symmetry. The spontaneous symmetry breaking in this model is chosen to obtain tribimaximal mixing in the neutrino sector. We introduce $Z_2 \times Z_2$ invariant perturbations…

高能物理 - 唯象学 · 物理学 2022-09-07 Abhish Dev , P. Ramadevi , S. Uma Sankar

To accommodate the recently observed non-zero reactor mixing angle $\theta_{13}$, we consider the lepton mixing matrix as Tri-bimaximal mixing (TBM) form in the leading order along with a perturbation in neutrino sector. The perturbation is…

高能物理 - 唯象学 · 物理学 2016-11-22 M. Sruthilaya , Srinu Gollu

We provide an explicit structure of the charged lepton mass matrix which is 2-3 symmetric except for a single breaking of this symmetry by the muon mass. We identify a flavor symmetric limit for the mass matrices where the first generation…

高能物理 - 唯象学 · 物理学 2012-02-22 Ahmed Rashed , Alakabha Datta

We point out two simple but instructive possibilities to construct the charged lepton and neutrino mass matrices, from which the nearly bi-maximal neutrino mixing with large T violation can naturally emerge. The two lepton mixing scenarios…

高能物理 - 唯象学 · 物理学 2014-11-17 Zhi-zhong Xing

We show that the Fritzsch texture of lepton mass matrices can naturally lead to the bi-large flavor mixing pattern, if three neutrinos have a normal but weak mass hierarchy (typically, $m_1 : m_2 : m_3 \sim 1 : 3 :10$). The effective mass…

高能物理 - 唯象学 · 物理学 2010-04-05 Zhi-zhong Xing
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