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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…

High Energy Physics - Phenomenology · Physics 2023-08-21 Aditya Batra , Praveen Bharadwaj , Sanjoy Mandal , Rahul Srivastava , José W. F. Valle

An explicit form of charged--lepton mass matrix, predicting $m_\tau = 1776.80$ MeV from the experimental values of $m_e$ and $m_\mu$ (in good agreement with the experimental figure $m_\tau = 1777.05^{+0.29}_{-0.26}$ MeV), is applied to…

High Energy Physics - Phenomenology · Physics 2007-05-23 Wojciech Krolikowski

In solar neutrino oscillations, if $\nu_e$ has a significant third massive component, the allowed parameter space in $\Delta m^2$ and $\sin^2 2 \theta$ for the first two components is shown to be greatly increased. This third component may…

High Energy Physics - Phenomenology · Physics 2007-05-23 Ernest Ma

We have investigated the lepton flavor violation in the supersymmetric framework assuming the large mixing angle MSW solution with the quasi-degenerate and the inverse-hierarchical neutrino masses. In the case of the quasi-degenerate…

High Energy Physics - Phenomenology · Physics 2009-11-07 A. Kageyama , S. Kaneko , N. Shimoyama , M. Tanimoto

We propose a new mechanism in which the generation of the supersymmetric $\mu $-term as well charged lepton masses is closely tied to R-parity violation involving heavy vector-like families . A realistic example based on $SU(3)_c\times…

High Energy Physics - Phenomenology · Physics 2008-12-18 Qaisar Shafi , Zurab Tavartkiladze

The current status of the physics of massive neutrinos is reviewed with a forward-looking emphasis. The article begins with the general phenomenology of neutrino oscillations in vacuum and matter and documents the experimental evidence for…

High Energy Physics - Phenomenology · Physics 2009-09-15 V. Barger , D. Marfatia , K. Whisnant

We discuss general predictions for neutrino masses and mixing angles from R parity violation in the Minimal Supersymmetric Standard Model. If the soft supersymmetry breaking terms are flavor blind at short distance, then the leptonic…

High Energy Physics - Phenomenology · Physics 2014-11-17 D. Elazzar Kaplan , Ann E. Nelson

Motivated by the Super-Kamiokande data, we revisit models with U(1) symmetries and discuss the origin of neutrino masses and mixings in such theories. We show that, in models with just three light neutrinos and a hierarchy of neutrino…

High Energy Physics - Phenomenology · Physics 2009-10-31 Smaragda Lola , Graham G. Ross

We suggest that the Large Mixing Angle MSW solar solution, whose unique physical status is confidently supported by the recent results from KamLAND experiments, gets its justification in the fermion universality, interpreted for neutrinos…

High Energy Physics - Phenomenology · Physics 2007-05-23 Wojciech Krolikowski

If the generating mechanism for neutrino mass is to account for both the newly observed muon anomalous magnetic moment as well as the present experimental bounds on lepton flavor nonconservation, then the neutrino mass matrix should be…

High Energy Physics - Phenomenology · Physics 2009-11-07 Ernest Ma , Martti Raidal

We show that the neutrino mixing pattern with the large mixing required for the atmospheric neutrino problem and the small mixing angle MSW solution for the solar neutrino problem can be naturally generated through radiative magnification,…

High Energy Physics - Phenomenology · Physics 2009-10-31 K. R. S. Balaji , Amol S. Dighe , R. N. Mohapatra , M. K. Parida

We revisit minimal non-supersymmetric models of SU(5) Grand Unification with the type II seesaw mechanism as the origin of neutrino masses. Imposing the requirement of gauge coupling unification and the proton lifetime bounds, we perform a…

High Energy Physics - Phenomenology · Physics 2022-12-02 Lorenzo Calibbi , Xiyuan Gao

The recent evidence for neutrino oscillations stimulate us to discuss again the problem of fermion masses and mixings in gauge theories. In the standard model, several forms for quark mass matrices are equivalent. They become ansatze within…

High Energy Physics - Phenomenology · Physics 2008-11-26 D. Falcone

Explicit expressions for the differential and total rates and emissivities of neutrino pairs from the photo-neutrino process $e^\pm + \gamma \to e^\pm + \nu + \bar\nu$ in hot and dense matter are derived. Full information about the emitted…

Astrophysics · Physics 2009-11-10 Sharada Iyer Dutta , Sasa Ratkovic , Madappa Prakash

Neutrinos stand out among elementary particles through their unusually small masses. Various seesaw mechanisms attempt to explain this fact. In this work applying insights from matrix theory we are in a position to treat variants of seesaw…

High Energy Physics - Phenomenology · Physics 2020-09-04 Wojciech Flieger , Janusz Gluza

We adopt a bottom-up approach to reconstruct the possible neutrino mass matrix patterns, in the hypothesis that $\lambda = \sin \theta_C$, where $\theta_C$ is the Cabibbo angle, is a useful expansion parameter in the neutrino sector as it…

High Energy Physics - Phenomenology · Physics 2010-09-14 Fu-Sin Ling

We apply the see-saw mechanism and an SO(10) model to neutrino masses and mixing in order to estimate the heavy Majorana masses. We discuss shortly the decay modes of heavy Majorana neutrinos and calculate their contribution to the lepton…

High Energy Physics - Phenomenology · Physics 2007-05-23 W. Alles , L. Frassinetti

A neutrino mass-mixing scheme which explains qualitatively all present evidence for neutrino mass (the solar and atmospheric neutrino deficits, LSND, and hot dark matter), and also makes possible heavy-element nucleosynthesis by supernovae,…

High Energy Physics - Phenomenology · Physics 2007-05-23 David O. Caldwell

We discuss Dirac neutrino masses and mixings in a scenario where both the standard model fermions and right handed neutrinos are bulk fields in a non-factorizable geometry in five dimensions. We show how the atmospheric and solar neutrino…

High Energy Physics - Phenomenology · Physics 2011-05-12 Stephan J. Huber , Qaisar Shafi

Assuming three flavour neutrino mixing takes place in vacuum, we investigate the possibility that the solar $\nu_e$ take part in MSW transitions in the Sun due to $\Delta m^2_{31} \sim (10^{-7} - 10^{-4})~eV^2$, followed by long wave length…

High Energy Physics - Phenomenology · Physics 2007-05-23 Qiu-Yu Liu