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相关论文: Neutrino masses through see-saw mechanism in 3-3-1…

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We propose a model for neutrino mass generation in wich no physics beyond a TeV is required. We extend the standard model by adding two charged singlet fields with lepton number two. Dirac neutrino masses $m_{\nu_D} \leq MeV$ are generated…

高能物理 - 唯象学 · 物理学 2009-11-07 Salah Nasri , Sherif Moussa

We investigate the see-saw mechanism for generally non-fine-tuned $n \times n$ mass matrices involving both Dirac and Majorana neutrinos. We specifically show that the number of naturally light neutrinos cannot exceed half of the dimension…

高能物理 - 唯象学 · 物理学 2009-11-07 Manfred Lindner , Tommy Ohlsson , Gerhart Seidl

The usual see-saw mechanism for the generation of light neutrino masses is based on the assumption that all of the flavours of right-handed (more properly, sterile) neutrinos are heavy. If the sterile Majorana mass matrix is singular, one…

高能物理 - 唯象学 · 物理学 2007-05-23 B. H. J. McKellar , G. J. Stephenson , T. Goldman , M. Garbutt

The effective Lagrangian for the seesaw model is derived including effects due to CP violation. Besides the usual dimension-5 operator responsible for light neutrino masses, a dimension-6 operator is obtained. For three or less heavy…

高能物理 - 唯象学 · 物理学 2008-11-26 A. Broncano , M. B. Gavela , E. Jenkins

In the extension of the standard model with one right-handed neutrino and one Higgs triplet, we propose a suppression mechanism, obtaining small masses for the active neutrinos, while mixing angles are predicted with a right-handed neutrino…

高能物理 - 唯象学 · 物理学 2018-10-12 R. Martinez , F. Ochoa , M. Ospina

The neutrino oscillations are studied in the framework of the minimal supersymmetric SO(10) model with Type-III see-saw mechanism by additionally introducing a number of SO(10) singlet neutrinos. The light Majorana neutrino mass matrix is…

高能物理 - 唯象学 · 物理学 2009-11-11 Takeshi Fukuyama , Amon Ilakovac , Tatsuru Kikuchi , Koichi Matsuda

We discuss a radiative type-I seesaw. In these models, the radiative generation of Dirac neutrino masses allows to explain the smallness of the observed neutrino mass scale for rather light right-handed neutrino masses in a type-I seesaw.…

高能物理 - 唯象学 · 物理学 2019-12-18 Carolina Arbeláez , A. E. Cárcamo Hernández , Ricardo Cepedello , Martin Hirsch , Sergey Kovalenko

We summarize the phenomenological constraints on seesaw scenarios defined at the TeV scale and provide a simple extension of the Standard Model which naturally leads to a testable mechanism of neutrino mass generation.

高能物理 - 唯象学 · 物理学 2013-12-19 Emiliano Molinaro

We propose a radiative seesaw model in alternative left-right model without any bidoublet scalar fields, in which all the fermion masses in the standard model are generated through a canonical seesaw mechanism at the tree level. On the…

高能物理 - 唯象学 · 物理学 2017-03-08 Takaaki Nomura , Hiroshi Okada , Yuta Orikasa

We implement the seesaw mechanism in the 3-3-1 model with right-handed neutrinos. This is accomplished by the introduction of a scalar sextet into the model and the spontaneous violation of the lepton number. We identify the Majoron as a…

高能物理 - 唯象学 · 物理学 2008-12-18 D. Cogollo , H. Diniz , C. A. de S. Pires , P. S. Rodrigues da Silva

A minimal extension of the Standard Model is proposed, where the observed left-handed neutrinos obtain naturally small Majorana masses from a one-loop radiative seesaw mechanism. This model has two candidates (one bosonic and one fermionic)…

高能物理 - 唯象学 · 物理学 2010-04-06 Ernest Ma

We prove that - even at a low TeV scale - the canonical seesaw mechanism can be naturally implemented in the exact solution of a particular 3-3-1 gauge model, since a very small alteration $\epsilon$ in the parameter matrix of the Higgs…

高能物理 - 唯象学 · 物理学 2009-08-01 Adrian Palcu

The compatibility of the Frobenius group T13 with the canonical see-saw mechanism of neutrino mixing is examined. The Standard Model is extended in a minimalist way, by introducing a family symmetry and three right-handed neutrinos. To fit…

高能物理 - 唯象学 · 物理学 2013-05-30 Christine Hartmann

A previous short analysis of the seesaw mechanism, based on quark-lepton symmetry, experimental data and hierarchical neutrino spectrum, is enlarged to include small but not zero U_{e3}, inverted mass hierarchy, and the qualitative effect…

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

The seesaw mechanism for three neutrinos is discussed, clarifying the situation where the seesaw texture results in three approximately zero mass eigenvalues. The true underlying mechanism is shown to be just the $inverse$ (or $linear$)…

高能物理 - 唯象学 · 物理学 2010-01-15 Xiao-Gang He , Ernest Ma

The linear seesaw mechanism provides a simple way to generate neutrino masses. In addition to Standard Model particles, it includes quasi-Dirac leptons as neutrino mass mediators, and a leptophilic scalar doublet seeding small neutrino…

高能物理 - 唯象学 · 物理学 2023-08-21 Aditya Batra , Praveen Bharadwaj , Sanjoy Mandal , Rahul Srivastava , José W. F. Valle

We discuss neutrino mass and mixing in the framework of the classic seesaw mechanism, involving right-handed neutrinos with large Majorana masses, which provides an appealing way to understand the smallness of neutrino masses. However, with…

高能物理 - 唯象学 · 物理学 2016-06-22 Stephen F. King

Experiments on neutrino oscillations have uncovered several small parameters, $\theta_{13}$ being a prominent one. Others are the solar mass splitting {\em vis-\`{a}-vis} the atmospheric one and the deviation of $\theta_{23}$ from maximal…

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

A novel scenario is presented within the Type-I seesaw mechanism in which no other beyond Standard Model fields except three heavy right handed neutrinos, have been considered. Light neutrino masses around sub eV scale, could be possible at…

高能物理 - 唯象学 · 物理学 2024-11-26 Kunal Pandey , Rathin Adhikari

The see-saw mechanism of neutrino mass generation may enhance lepton mixing up to maximal even if the Dirac mass matrices of leptons have structure similar to that in the quark sector. Two sets of conditions for such an enhancement are…

高能物理 - 唯象学 · 物理学 2009-10-22 Alexei Yu. Smirnov