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Despite being very successful in explaining the wide range of precision experimental results obtained so far, the Standard Model (SM) of elementary particles fails to address two of the greatest observations of the recent decades: tiny but…

高能物理 - 唯象学 · 物理学 2010-11-19 Yasaman Farzan , Silvia Pascoli , Michael A. Schmidt

We propose a flavour theory in which the family symmetry results naturally from a six-dimensional orbifold compactification. "Diracness" of neutrinos is a consequence of the spacetime dimensionality, and the fact that right-handed neutrinos…

高能物理 - 唯象学 · 物理学 2020-11-03 Francisco J. de Anda , Ignatios Antoniadis , José W. F. Valle , Carlos A. Vaquera-Araujo

We analyze a model with unbroken B-L gauge symmetry where neutrino masses are generated at one loop, after spontaneous breaking of a global U(1) symmetry. These symmetries ensure dark matter stability and the Diracness of neutrinos. Within…

高能物理 - 唯象学 · 物理学 2021-05-14 Carlos Alvarado , Cesar Bonilla , Julio Leite , José W. F. Valle

We present a supersymmetric model of dark energy from Mass Varying Neutrinos which is stable against radiative corrections to masses and couplings, and free of dynamical instabilities. This is the only such model of dark energy involving…

高能物理 - 唯象学 · 物理学 2009-11-11 Rob Fardon , Ann E. Nelson , Neal Weiner

The specific violated mirror symmetry model is capable of generating the observed lepton weak mixing matrix with a structure similar to the observed one that almost lacks any visible regularities (the "flavor riddle"). The peculiarities of…

高能物理 - 唯象学 · 物理学 2017-09-13 Igor T. Dyatlov

We present a TeV scale seesaw mechanism for exploring the dark matter and neutrino phenomenology in the light of recent neutrino and cosmology data. A different realization of the Inverse seesaw(ISS) mechanism with $A_{4}$ flavor symmetry…

高能物理 - 唯象学 · 物理学 2016-10-20 Ananya Mukherjee , Mrinal Kumar Das

We suggest that recent neutrino puzzles that are the solar and atmospheric neutrino deficits as well as the possible neutrino oscillations reported by the LSND experiment and the possibility of massive neutrinos providing the hot component…

高能物理 - 唯象学 · 物理学 2009-10-28 Z. Berezhiani , R. N. Mohapatra

The nature of dark matter is one of the open problems of the Standard Model of particle physics. Despite the great experimental efforts, we have not yet found a positive signal of its interactions with ordinary matter. One possible…

高能物理 - 唯象学 · 物理学 2019-04-09 M. Blennow , E. Fernández-Martínez , A. Olivares-Del Campo , S. Pascoli , S. Rosauro-Alcaraz , A. V. Titov

As is well-known, if the scattering cross section of the Dark Matter (DM) particles off the nuclei inside the Sun is large enough, the Sun can trap DM particles. In principle, the annihilation of DM pair inside the Sun can then lead to the…

高能物理 - 唯象学 · 物理学 2015-06-03 Yasaman Farzan

Seesaw models with leptonic symmetries allow right-handed (RH) neutrino masses at the electroweak scale, or even lower, at the same time having large Yukawa couplings with the Standard Model leptons, thus yielding observable effects at…

高能物理 - 唯象学 · 物理学 2016-12-30 Lucien Heurtier , Daniele Teresi

We discuss the possibility of flavor symmetries to explain the pattern of charged lepton and neutrino masses and mixing angles. We emphasize what are the obstacles for the generation of an almost maximal atmospheric mixing and what are the…

高能物理 - 唯象学 · 物理学 2014-11-17 Shao-Long Chen , Michele Frigerio , Ernest Ma

A new framework for handling flavor symmetry breaking in the neutrino sector is discussed where the source of symmetry breaking is traced to the global property of right-handed neutrinos in extra-dimensional space. Light neutrino…

高能物理 - 唯象学 · 物理学 2009-11-11 Naoyuki Haba , Atsushi Watanabe , Koichi Yoshioka

The origin of neutrino mass is a mystery, so is its nature, namely, whether neutrinos are Dirac or Majorana particles. On top of that, hints of large deviations of the muon and the electron anomalous magnetic moments (AMMs) are strong…

高能物理 - 唯象学 · 物理学 2022-09-07 Talal Ahmed Chowdhury , Md. Ehsanuzzaman , Shaikh Saad

We construct a flavor symmetry model based on the tetrahedral group A_4 in which the right-handed neutrinos from the seesaw mechanism can be both keV warm dark matter particles and eV-scale sterile neutrinos. This is achieved by giving the…

高能物理 - 唯象学 · 物理学 2012-02-01 James Barry , Werner Rodejohann , He Zhang

We study the implications of a large nu_mu - nu_tau mixing angle on flavour changing transitions of quarks and leptons in supersymmetric extensions of the standard model. Two patterns of supersymmetry breaking are considered, models with…

高能物理 - 唯象学 · 物理学 2014-11-17 Wilfried Buchmuller , David Delepine , Laksana Tri Handoko

A minimal extension of the Standard Model (SM) featuring two scalar leptoquarks, an SU(2) doublet with hypercharge 1/6 and a singlet with hypercharge 1/3, is proposed as an economical benchmark model for studies of an interplay between…

高能物理 - 唯象学 · 物理学 2023-11-13 Felipe F. Freitas , João Gonçalves , António P. Morais , Roman Pasechnik , Werner Porod

The scattering of neutrinos off dark matter can induce time delays in their propagation compared to that of photons, which would wash out correlations between ultra-high-energy neutrinos and electromagnetic observations of their sources -…

高能物理 - 唯象学 · 物理学 2019-09-11 Seth Koren

We present a model that extends the standard model by incorporating the simplest discrete symmetry groups, $Z_2$ and $Z_3$. This model introduces vector-like leptons and a real scalar singlet. Based on this framework, we generate Dirac…

高能物理 - 唯象学 · 物理学 2025-08-20 Yakefu Reyimuaji , Murat Abdughani

Flavour physics represents one of the most interesting and, at the same time, less understood sector of the Standard Theory. On the one hand, the peculiar pattern of quark and lepton masses, and their mixing angles, may be the clue to some…

高能物理 - 唯象学 · 物理学 2016-10-12 Gino Isidori

Cold dark matter explains a wide range of data on cosmological scales. However, there has been a steady accumulation of evidence for discrepancies between simulations and observations at scales smaller than galaxy clusters. Solutions to…

高能物理 - 唯象学 · 物理学 2014-12-11 Bridget Bertoni , Seyda Ipek , David McKeen , Ann E. Nelson