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相关论文: Summary of Model Predictions for $U_{e3}$

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We present a model of neutrino masses combining the seesaw mechanism and strong Dirac mass hierarchy and at the same time exhibiting a significantly reduced hierarchy at the level of active neutrino masses. The heavy Majorana masses are…

高能物理 - 唯象学 · 物理学 2007-05-23 M. Jezabek , P. Urban

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 mixing of three and four massive neutrinos is considered. It is shown that the neutrino oscillation data are not compatible with a hierarchy of couplings in the three-neutrino case. In the case of four neutrinos, a hierarchy of masses…

高能物理 - 唯象学 · 物理学 2007-05-23 S. M. Bilenky , C. Giunti , W. Grimus

In spite of enormous experimental progress in determination of the neutrino parameters, theory of neutrino mass and mixing is still on the cross-roads. Guidelines could be (i) the connection between zero neutrino charges (and therefore a…

高能物理 - 唯象学 · 物理学 2022-03-02 Alexei Yu. Smirnov

A new type of neutrino mixing named bi-pair neutrino mixing is proposed to describe the current neutrino mixing pattern with a vanishing reactor mixing angle and is determined by a mixing matrix with two pairs of identical magnitudes of…

高能物理 - 唯象学 · 物理学 2011-02-11 Teruyuki Kitabayashi , Masaki Yasue

We review the current status of the neutrino mass and mixing parameters needed to reconstruct the neutrino mass matrix. A comparative study of the precision in the measurement of oscillation parameters expected from the next generation…

高能物理 - 唯象学 · 物理学 2016-09-06 Sandhya Choubey

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 study the effects of breaking S3 symmetry in the neutrino mass matrix for the masses and mixing matrix of neutrinos. At zeroth order the model gives degenerate neutrino masses and accommodates tribimaximal mixing. We introduce…

高能物理 - 唯象学 · 物理学 2012-02-16 S. Dev , Radha Raman Gautam , Lal Singh

Many experiments are currently looking for evidence of neutrino mass in the form of neutrino oscillations. Oscillation probabilities are non-linear functions of the neutrino mixing matrix elements, so most comparisons of data to theory are…

高能物理 - 唯象学 · 物理学 2007-05-23 Doris Jeanne Wagner

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

It is argued that the observed vacuum energy density and the small values of the neutrino masses could be due to anthropic selection effects. Until now, these two quantities have been treated separately from each other and, in particular,…

天体物理学 · 物理学 2009-10-07 Levon Pogosian , Alexander Vilenkin , Max Tegmark

In this lecture we review some of the basic properties of neutrinos, in particular their mass and the oscillation behavior. First we discuss how to describe the neutrino mass. Then, under the assumption that neutrinos are massive and mixed,…

高能物理 - 唯象学 · 物理学 2007-05-23 C. W. Kim

The recent progress in establishing the existence of finite neutrino masses and mixing between generations of neutrinos has been remarkable, if not astounding. The combined results from studies of atmospheric neutrinos, solar neutrinos, and…

高能物理 - 唯象学 · 物理学 2011-07-19 R. D. McKeown , P. Vogel

In a recent paper [1] we showed that, assuming no fine tuning between certain elements of the neutrino mass matrix, one can link the element U_{e3} of the lepton mixing matrix to solar and atmospheric neutrino oscillation parameters. This…

高能物理 - 唯象学 · 物理学 2007-05-23 E. Kh. Akhmedov , G. C. Branco , M. N. Rebelo

We propose a novel theoretical understanding of neutrino masses and mixings, which is attributed to the intrinsic vector-like feature of the regularized Standard Model at short distances. We try to explain the smallness of Dirac neutrino…

高能物理 - 唯象学 · 物理学 2014-11-17 She-Sheng Xue

The mass estimates of active and sterile (right-handed) neutrinos are considered at the phenomenological level using the seesaw mechanism. It is assumed that the neutrino mass values depend on three characteristic scales, and the sum of the…

高能物理 - 唯象学 · 物理学 2025-05-13 V. V. Khruschov , S. V. Fomichev

After a brief introduction to neutrino mass via the see-saw model I discuss neutrino mixing and oscillation, first in vacuum and then its matter enhancement. Then the solar and atmospheric neutrino oscillation data are briefly reviewed.…

高能物理 - 唯象学 · 物理学 2009-10-31 D. P. Roy

We investigate the tree-level neutrino mass generation in the gauged $U(1)_\ell$ lepton model recently proposed by us [arXiv:1805.10382]. With the addition of one Standard Model(SM) singlet, $\phi_1(Y=0, \ell=1)$, and one SM triplet scalar,…

高能物理 - 唯象学 · 物理学 2018-10-05 We-Fu Chang , John N. Ng

Neutrino oscillations are now a well-stablished and deeply studied phenomena. Their mixing parameters, except for the CP phase, are measured with good accuracy. The three-neutrino oscillation picture in matter is currently of great interest…

高能物理 - 唯象学 · 物理学 2016-03-02 L. J. Flores , O. G. Miranda

We determine the neutrino mixing and mass parameters that are allowed by the Super-Kamiokande atmospheric neutrino data in a three-neutrino model with one mass-squared difference contributing to the oscillations. We find that although…

高能物理 - 唯象学 · 物理学 2009-09-15 V. Barger , T. J. Weiler , K. Whisnant