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相关论文: Modified Zee mass matrix with zero-sum condition

200 篇论文

Working in the framework of three chiral neutrinos with Majorana masses, we investigate a scenario first realized in an explicit model by Zee: that the neutrino mass matrix is strictly off-diagonal in the flavor basis, with all its diagonal…

高能物理 - 唯象学 · 物理学 2009-10-31 Paul H. Frampton

The Zee model, which employs the standard Higgs scalar ($\phi$) with its duplicate ($\phi^\prime$) and a singly charged scalar ($h^+$), can utilize two global symmetries associated with the conservation of the numbers of $\phi$ and…

高能物理 - 唯象学 · 物理学 2014-11-17 Teruyuki Kitabayashi , Masaki Yasue

It is well known that Zee type neutrino mass matrix can provide bi-maximal neutrino mixing for three neutrinos. We study the reconciliation of this model with the gauge mediated supersymmetry breaking scenario, which naturally suppresses…

高能物理 - 唯象学 · 物理学 2008-11-26 N. Haba , M. Matsuda , M. Tanimoto

We study the possible manifestation of the interference between the effects produced in the atmospheric neutrinos due to oscillation driven by the solar parameters parameters $\Delta m^2_{21}$, $\sin^2 2\theta_{21}$ and due to oscillation…

高能物理 - 唯象学 · 物理学 2015-06-25 O. L. G. Peres , A. Yu. Smirnov

We propose simple phenomenological lepton mass matrices which describe the three neutrinos almost degenerate in mass, leading to a very large mixing angle between $\nu_\mu$ and $\nu_\tau$, as consistent with a recent report on atmospheric…

高能物理 - 唯象学 · 物理学 2009-10-30 M. Fukugita , M. Tanimoto , T. Yanagida

Neutrino oscillations reveal several small parameters, namely, $\theta_{13}$, the solar mass splitting {\em vis-\`{a}-vis} the atmospheric one, and the deviation of $\theta_{23}$ from maximal mixing. Can these small quantities all be traced…

高能物理 - 唯象学 · 物理学 2015-05-27 Soumita Pramanick , Amitava Raychaudhuri

A simple unifying mass matrix is presented for the three active and one sterile neutrinos $\nu_e$, $\nu_\mu$, $\nu_\tau$ and $\nu_s$, using an extension of the radiative mechanism proposed some time ago by Zee. The total…

高能物理 - 唯象学 · 物理学 2009-01-01 Naveen Gaur , Ambar Ghosal , Ernest Ma , Probir Roy

Neutrino mass matrix generated by the Zee (radiative) mechanism has zero (in general, small) diagonal elements and a natural hierarchy of the nondiagonal elements. It can be considered as an alternative (with strong predictive power) to the…

高能物理 - 唯象学 · 物理学 2009-10-28 Alexei Yu. Smirnov , Zhijian Tao

A simple 3 X 3 neutrino mass matrix is proposed to accommodate both the solar and atmospheric neutrino deficits. This scenario can be realized naturally by a radiative mechanism for the generation of neutrino masses. It also goes together…

高能物理 - 唯象学 · 物理学 2010-01-06 Ernest Ma

Results of a new analysis of the CHOOZ data, performed in the framework of three-neutrino mixing, are presented. Both the cases of normal and inverted neutrino mass hierarchy are considered. The parameters characterizing the solar neutrino…

高能物理 - 唯象学 · 物理学 2015-06-25 S. M. Bilenky , D. Nicolo , S. T. Petcov

We systematically analyze the radiative corrections to the $S_3$ symmetric neutrino mass matrix at high energy scale, say the GUT scale, in the charged lepton basis. There are significant corrections to the neutrino parameters both in the…

高能物理 - 唯象学 · 物理学 2015-06-22 Shivani Gupta , C. S. Kim , Pankaj Sharma

Inspired by the neutrino oscillations data, we consider the exact $\mu-\tau$ symmetry, implemented at the level of the neutrino mass matrix, as a good initial framework around which to study and describe neutrino phenomenology. Working in…

高能物理 - 唯象学 · 物理学 2021-07-14 N. Chamoun , C. Hamzaoui , S. Lashin , S. Nasri , M. Toharia

We investigate neutrino masses and mixings within the framework of the Zee mass matrix, with three lepton flavors. It is shown that the bi-maximal solution is the only possibility to reconcile atmospheric and solar neutrino data, within…

高能物理 - 唯象学 · 物理学 2009-10-31 C. Jarlskog , M. Matsuda , S. Skadhauge , M. Tanimoto

We know $L_e-L_\mu-L_\tau$ symmetry gives $m^2_1= m^2_2 >> m^2_3$ pattern in Zee model. $\Delta m^2_\odot$ emerges from a small breaking of this symmetry. Because this symmetry is broken very weakly $\theta_\odot$ does not deviate much from…

高能物理 - 唯象学 · 物理学 2009-11-07 Biswajoy Brahmachari , Sandhya Choubey

The eigenvalues and mixing angles in the Zee model are investigated parameter-independently. When we require |\Delta m^2_{12}/\Delta m^2_{23}| \ll 1 in order to understand the solar and atmospheric data simultaneously, the only solution is…

高能物理 - 唯象学 · 物理学 2009-11-07 Yoshio Koide

Assuming the solar and atmospheric neutrino deficits to be due to neutrino oscillations, it is shown that the 3X3 mass matrix spanning the e, mu, and tau neutrinos may have already revealed a seesaw mass pattern. Also, this matrix is the…

高能物理 - 唯象学 · 物理学 2016-09-01 Ernest Ma , J. Pantaleone

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 present a Zee model with a family dependent $Z_2$ symmetry for radiative neutrino masses. Our motivation is to get a model that correctly describes neutrino oscillation phenomena, while at the same time offers definite predictions. The…

高能物理 - 唯象学 · 物理学 2022-03-29 R. Primulando , J. Julio , P. Uttayarat

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 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