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Related papers: Neutrino mass generation in asymptotically safe gr…

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Neutrino masses and mixings are investigated on the basis of a universal seesaw mass matrix model, in which quark (except for top) and charged lepton mass matrices M_f and neutrino mass matrix M_\nu are given by M_f \simeq m_L M_F^{-1} m_R…

High Energy Physics - Phenomenology · Physics 2009-10-30 Yoshio Koide

We study a model where the Standard Model is augmented with three sterile neutrinos. By adopting a particular parameterization of a $(6\times6)$ unitary matrix - in this context, light neutrino masses being generated via a type-I seesaw…

High Energy Physics - Phenomenology · Physics 2024-07-17 Debashree Priyadarsini Das , Sasmita Mishra

We consider the extension of the Standard Model (SM) with a strongly interacting QCD-like hidden sector, at least two generations of right-handed neutrinos and one scalar singlet. Once scalar singlet obtains a nonzero vacuum expectation…

High Energy Physics - Phenomenology · Physics 2020-08-28 Mayumi Aoki , Vedran Brdar , Jisuke Kubo

We study the neutrino mass generation in the $SU(4)_L \otimes U(1)_X$ electroweak extension of the standard model by considering non-renormalizable dimension five effective operators. It is shown that there exist two topologies for the…

High Energy Physics - Phenomenology · Physics 2016-09-09 Guillermo Palacio

In Gravity Unified Theories all operators that are consistent with the local gauge and discrete symmetries are expected to arise in the effective low-energy theory. Given the absence of multiplets like 126 of SO(10) in string models, and…

High Energy Physics - Phenomenology · Physics 2016-09-06 Alon E. Faraggi , Jogesh Pati

We investigate the impact of prior models on the upper bound of the sum of neutrino masses, $\sum m_{\nu}$. We use data from Large Scale Structure of galaxies, Cosmic Microwave Background, Type Ia SuperNovae, and Big Bang Nucleosynthesis.…

It is usually believed that the observation of the neutrino-antineutrino (${\nu}$-$\bar{\nu}$) oscillations is almost impossible since the oscillation probabilities are expected to be greatly suppressed by the square of tiny ratio of…

High Energy Physics - Phenomenology · Physics 2017-04-05 Chao-Qiang Geng , Da Huang

Motivated by recent results from neutrino experiments, we study the neutrino masses and mixing in the framework of a SUSY $SU(5)\times \mathbb{A}_{4} $ model. The hybrid of Type I and Type II seesaw mechanisms leads to the nonzero value of…

High Energy Physics - Phenomenology · Physics 2018-07-11 R. Ahl Laamara , M. A. Loualidi , M. Miskaoui , E. H. Saidi

Explaining the tiny neutrino masses and non-zero mixings have been one of the key motivations for going beyond the framework of the Standard Model (SM). We discuss a collider testable model for generating neutrino masses and mixings via…

High Energy Physics - Phenomenology · Physics 2020-07-06 Avnish , Kirtiman Ghosh

The see-saw mechanism is usually applied to explain the lightness of neutrinos. The traditional see-saw mechanism introduces at least two right-handed neutrinos for the realistic neutrino spectrum. In the case of supersymmetry, loop…

High Energy Physics - Phenomenology · Physics 2014-12-01 Yi-Lei Tang

This is a review article about neutrino mass models, particularly see-saw models involving three active neutrinos which are capable of describing both the atmospheric neutrino oscillation data, and the large mixing angle MSW solar solution,…

High Energy Physics - Phenomenology · Physics 2009-11-10 S. F. King

We propose a supersymmetric extra U(1) model, which can generate small neutrino masses and necessary $\mu$ terms, simultaneously. Fields including quarks and leptons are embedded in three ${\bf 27}$s of $E_6$ in a different way among…

High Energy Physics - Phenomenology · Physics 2014-11-20 Daijiro Suematsu , Takashi Toma , Tetsuro Yoshida

Our knowledge of the neutrino sector of the Standard Model has recently undergone a revolution. Deficits of the atmospheric muon neutrino flux and the solar electron neutrino flux compared to their predicted values can be understood in…

High Energy Physics - Phenomenology · Physics 2009-10-31 V. Barger

In this work we show that we can generate neutrino masses through the type-II see-saw mechanism working at TeV scale in the context of a 331 model.

High Energy Physics - Phenomenology · Physics 2014-11-17 J. C. Montero , C. A. de S. Pires , V. Pleitez

The neutrino mass generation mechanism, the nature of dark matter and the origin of the baryon asymmetry of the Universe are three compelling questions that cannot be accounted for in the Standard Model of particle physics. In this thesis…

High Energy Physics - Phenomenology · Physics 2016-09-23 Michele Lucente

In pursuit of a balance between theoretical naturalness and experimental testability, we propose two classes of multiple seesaw mechanisms at the TeV scale to understand the origin of tiny neutrino masses. They are novel extensions of the…

High Energy Physics - Phenomenology · Physics 2009-09-28 Zhi-zhong Xing , Shun Zhou

After outlining some popular ways to go beyond the standard model so as to generate non-zero but tiny neutrino masses, I focus on several typical seesaw mechanisms and discuss how to get a balance between their theoretical naturalness and…

High Energy Physics - Phenomenology · Physics 2011-04-15 Zhi-zhong Xing

Previous fits of sterile neutrino dark matter models to cosmological data assumed a peculiar production mechanism, which is not representative of the best-motivated particle physics models given current data on neutrino oscillations. These…

High Energy Physics - Phenomenology · Physics 2009-06-30 Alexey Boyarsky , Julien Lesgourgues , Oleg Ruchayskiy , Matteo Viel

The mass-varying neutrino scenario is analyzed for three trial quintessence potentials (Ferreira-Joyce, inverse exponential, and thawing oscillating). The neutrino mass is generated via Yukawa coupling to the scalar field which represents…

High Energy Physics - Phenomenology · Physics 2021-05-19 Sayan Mandal , Gennady Y. Chitov , Olga Avsajanishvili , Bijit Singha , Tina Kahniashvili

There are many hints that gravity is asymptotically safe. The inclusion of gravitational corrections can result in the ultraviolet fundamental Standard Model and constrain the Higgs mass to take the smallest value such that electroweak…

High Energy Physics - Phenomenology · Physics 2019-12-11 Jan H. Kwapisz