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相关论文: Is Zee Model The Model of Neutrino Masses?

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The original Zee model can easily accommodate a bi-maximal mixing solution for the atmospheric and solar neutrino problems. From the most recent fit to the data we obtain a set of parameters for the Zee model. However, the recent claim on a…

高能物理 - 唯象学 · 物理学 2007-05-23 Ming-Yang Cheng , Kingman Cheung

We discuss an extended $SU(2)\times U(1)$ model which naturally leads to mass scales and mixing angles relevant for understanding both the solar and atmospheric neutrino anomalies. No right-handed neutrinos are introduced in the model.The…

高能物理 - 唯象学 · 物理学 2009-10-31 Anjan S. Joshipura , Saurabh D. Rindani

Evidence for neutrino oscillations is pointing to the existence of tiny but finite neutrino masses. Such masses may be naturally generated via radiative corrections in models such as the Zee model where a singlet Zee-scalar plays a key…

高能物理 - 唯象学 · 物理学 2009-11-07 Duane A. Dicus , Hong-Jian He , John N. Ng

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

The combined requirements, of (i) a natural solution to the fermion mass hierarchy problem and (ii) an explanation of both the atmospheric and solar neutrino problems, lead to an essentially unique picture of neutrino masses and mixing…

高能物理 - 唯象学 · 物理学 2009-10-30 C. D. Froggatt , M. Gibson , H. B. Nielsen

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

The three neutrino Zee model and its extension including three active and one sterile species are studied in the light of new neutrino oscillation data. We obtain analytical relations for the mixing angle in solar oscillations in terms of…

高能物理 - 唯象学 · 物理学 2009-11-07 Probir Roy , Sudhir K. Vempati

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

The inert Zee model is an extension of the Zee model for neutrino masses to allow for a solution to the dark matter problem that involves two vector-like fields, a doublet and a singlet of ${\rm SU(2)_L}$, and two scalars, also a doublet…

高能物理 - 唯象学 · 物理学 2018-11-27 Robinson Longas

The Zee model generates neutrino masses at the one-loop level by adding charged SU(2)_L-singlet and extra SU(2)_L-doublet scalars to the standard model of particle physics. As the origin of the nontrivial structure of the lepton flavor…

高能物理 - 唯象学 · 物理学 2015-03-17 Takeshi Fukuyama , Hiroaki Sugiyama , Koji Tsumura

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

Theories with large extra dimensions can generate small neutrino masses when the standard model neutrinos are coupled to singlet fermions propagating in higher dimensions. The couplings can also generate mass splittings and mixings among…

高能物理 - 唯象学 · 物理学 2009-11-07 Amol S. Dighe , Anjan S. Joshipura

We examine the neutrino mass matrix in the version of Zee model where both Higgs doublets couple to the leptons. We show that in this case one can accommodate the large mixing angle (LMA) MSW solution of the solar neutrino problem, while…

高能物理 - 唯象学 · 物理学 2009-11-07 K. R. S. Balaji , W. Grimus , T. Schwetz

We follow a minimalistic approach to neutrino masses, by introducing a single heavy singlet $N$ into the standard model (or supersymmetric standard model) with a heavy Majorana mass $M$, which couples as a single right-handed neutrino in a…

高能物理 - 唯象学 · 物理学 2009-10-31 S. F. King

It is shown that the bi-maximal solution is the only possibility to reconcile Zee-type neutrino mass matrix with three flavors to the current atmospheric and solar neutrino experimental data. The mass of the lightest neutrino, which consist…

高能物理 - 唯象学 · 物理学 2007-05-23 M. Matsuda , C. Jarlskog , S. Skadhauge , M. Tanimoto

We study a realization of the topology of the Zee model for the generation of neutrino masses at one-loop with a minimal set of vector-like fermions. After imposing an exact $Z_2$ symmetry to avoid tree-level Higgs-mediated flavor changing…

高能物理 - 唯象学 · 物理学 2016-05-04 Robinson Longas , Dilia Portillo , Diego Restrepo , Oscar Zapata

The radiative model, proposed by Zee, is extended from the three neutrino $(\nu_{e,\mu,\tau})$ sector to include a fourth sterile neutrino $\nu_s$. The oscillations $\nu_e \leftrightarrow \nu_s$ (solar), $\nu_\mu \leftrightarrow \nu_\tau$…

高能物理 - 唯象学 · 物理学 2007-05-23 Probir Roy

The CDF collaboration at Fermilab has recently reported a new precision measurement of the $W$~boson mass showing a substantial $7\sigma$ deviation from the Standard Model prediction. Moreover, Fermilab has recently confirmed the…

高能物理 - 唯象学 · 物理学 2022-08-17 Talal Ahmed Chowdhury , Julian Heeck , Shaikh Saad , Anil Thapa

The atmospheric and solar neutrino oscillation data suggest hierarchical neutrino masses with at least one large mixing. The simplest see-saw models for reconciling the two features are U(1) extensions of the SM with flavour dependent gauge…

高能物理 - 唯象学 · 物理学 2009-10-31 D. P. Roy
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