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相关论文: Prediction of $U_{e3}$ in Neutrino Mass Matrix wit…

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After the successful determination of the reactor neutrino mixing angle \theta_13 ~ 0.16 \neq 0, a new feature suggested by the current neutrino oscillation data is a sizeable deviation of the atmospheric neutrino mixing angle \theta_23…

高能物理 - 唯象学 · 物理学 2014-01-30 David Marzocca , Serguey T. Petcov , Andrea Romanino , Maria C. Sevilla

It is shown that the neutrino mass matrices in the flavour basis yielding a vanishing $U_{e3}$ are characterized by invariance under a class of $Z_2$ symmetries. A specific $Z_2$ in this class also leads to a maximal atmospheric mixing…

高能物理 - 唯象学 · 物理学 2016-08-16 Walter Grimus , Anjan S. Joshipura , Satoru Kaneko , Luís Lavoura , Hideyuki Sawanaka , Morimitsu Tanimoto

We consider the possibility to gain information on the lepton mixing matrix element |U_{e3}| from an improved experimental limit on the effective neutrino mass governing neutrino-less double beta decay. We show that typically a lower limit…

高能物理 - 唯象学 · 物理学 2009-12-17 Alexander Merle , Werner Rodejohann

We consider corrections to vanishing U_{e3} and maximal atmospheric neutrino mixing originating from the relation U = U_ell^dagger U_nu, where U is the PMNS mixing matrix and U_ell (U_nu) is associated with the diagonalization of the…

高能物理 - 唯象学 · 物理学 2008-11-26 K. A. Hochmuth , S. T. Petcov , W. Rodejohann

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

We give minimal values for the smallest lepton mixing parameter U_{e3}, applying 2-loop renormalization group equations in an effective theory approach. This is relevant in scenarios that predict an inverted neutrino mass spectrum with the…

高能物理 - 唯象学 · 物理学 2011-02-11 Shamayita Ray , Werner Rodejohann , Michael A. Schmidt

It has been said that the measurements of $U_{e3}$ in the lepton flavor mixing matrix would help discriminate between the possible solar neutrino solutions under the natural conditions with the neutrino mass hierarchies of $m_1 \ll m_2 \ll…

高能物理 - 唯象学 · 物理学 2009-10-31 N. Haba , Tomoharu Suzuki

We have discussed the impact of $U_{e3}$ on the model of the neutrino mass matrix. In order to get the small $U_{e3}$, some flavor symmetry is required. Typical two models are investigated. The first one is the model in which the bi-maximal…

高能物理 - 唯象学 · 物理学 2017-08-23 Morimitsu Tanimoto

As neutrino experiments are starting to probe the detailed structure of the neutrino mass matrix, we present sumrules relating its matrix elements for a class of models with approximate $L_e-L_{\mu}-L_{\tau}$ symmetry and the observables in…

高能物理 - 唯象学 · 物理学 2015-06-25 H. S. Goh , R. N. Mohapatra , S. -P. Ng

We point out that determination of the MNS matrix element |U_{e3}| = s_{13} in long-baseline \nu_{\mu} \to \nu_e neutrino oscillation experiments suffers from large intrinsic uncertainty due to the unknown CP violating phase \delta and sign…

高能物理 - 唯象学 · 物理学 2009-11-07 Takaaki Kajita , Hisakazu Minakata , Hiroshi Nunokawa

An approximate Z_3 family symmetry is proposed for leptons which results in a neutrino mass matrix with sin^2 2 theta_atm = 1 and tan^2 theta_sol = 0.5, but the latter value could easily be smaller. A generic requirement of this approach is…

高能物理 - 唯象学 · 物理学 2007-05-23 Ernest Ma

We point out under the assumption of Majorana neutrinos that a lower bound on the MNS matrix element |U_{e3}|^2 can be derived by using constraint imposed by neutrinoless double beta decay experiments and by positive detection of neutrino…

高能物理 - 唯象学 · 物理学 2009-11-07 Hisakazu Minakata , Hiroaki Sugiyama

We consider the possibility of neutrinos being Dirac particles and study minimal mass matrices with as much zero entries as possible. We find that up to 5 zero entries are allowed. Those matrices predict one vanishing mass state, CP…

高能物理 - 唯象学 · 物理学 2010-02-03 C. Hagedorn , W. Rodejohann

The A_4 model of leptons was proposed originally for nearly degenerate neutrino masses. With minimal modification, it is shown to accommodate as well the cases of normal hierarchy and inverted hierarchy. In all cases, this new model…

高能物理 - 唯象学 · 物理学 2009-11-10 Ernest Ma

We motivate the simplest ansatz for the neutrino mass matrix consistent with the data from neutrino oscillation experiments, and admitting CP violation. It has only two free parameters: an arbitrary mass-scale and a small dimensionless…

高能物理 - 唯象学 · 物理学 2010-04-05 P. F. Harrison , W. G. Scott

We have studied how observables of the neutrino mixing matrix can link up with the ones in the quark sector. The deviation from the bi-maximal flavor mixing is parameterized using a 3 x 3 unitary matrix. The neutrino mixings are…

高能物理 - 唯象学 · 物理学 2009-11-07 C. Giunti , M. Tanimoto

We make a general study of possibility of generating solar scale $\Delta_{\odot}$ and the CHOOZ angle $U_{e3}$ radiatively by assuming that they are zero at some high scale. The most general neutrino mass matrix leading to this result is…

高能物理 - 唯象学 · 物理学 2014-11-17 Anjan S. Joshipura

We propose two phenomenological scenarios of lepton mass matrices and show that either of them can exactly give rise to \tan^2\theta_{13} = m_e/(m_e + 2m_\mu), \tan^2\theta_{23} = m_\mu/(m_e + m_\mu) and \tan^2\theta_{12} = (m_e m_2 +…

高能物理 - 唯象学 · 物理学 2010-02-17 Harald Fritzsch , Zhi-zhong Xing

Motivated by recent measurements which strongly support a nonzero reactor mixing angle $\theta_{13}$, we study a deviation from $S_3$ neutrino discrete symmetry by explicitly breaking the neutrino mass matrix with a general retrocirculant…

高能物理 - 唯象学 · 物理学 2013-08-13 H. B. Benaoum

After some preliminary arguments suggesting that neutrino mixings with inverted mass pattern may be easier to understand within the framework of a local horizontal symmetry SU(2)_H acting on leptons, we construct a specific extension of the…

高能物理 - 唯象学 · 物理学 2014-11-17 R. Kuchimanchi , R. N. Mohapatra
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