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相关论文: New Neutrino Physics Without Fine Tuning

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In theories with a low quantum gravity scale, global symmetries are expected to be violated, inducing excessive proton decay or large Majorana neutrino masses. The simplest cure is to impose discrete gauge symmetries, which in turn make…

高能物理 - 唯象学 · 物理学 2009-09-29 Hooman Davoudiasl , Ryuichiro Kitano , Graham D. Kribs , Hitoshi Murayama

Standard Model predictions for neutrino-electron scattering cross-sections, including effects of electroweak radiative corrections, are reviewed. The sensitivity of those quantities to neutrino dipole moments, z' bosons, dynamical symmetry…

高能物理 - 唯象学 · 物理学 2008-11-26 William J. Marciano , Zohreh Parsa

Scale invariance may be a classical symmetry which is broken radiatively. This provides a simple way to stabilize the scale of electroweak symmetry breaking against radiative corrections. The simplest phenomenologically successful model of…

高能物理 - 唯象学 · 物理学 2008-11-26 Robert Foot , Archil Kobakhidze , Kristian. L. McDonald , Raymond. R. Volkas

A brief sketch is made of the present observational status of neutrino physics, with emphasis on the hints that follow from solar and atmospheric neutrino observations, as well as cosmological data on the amplitude of primordial density…

高能物理 - 唯象学 · 物理学 2009-09-17 J. W. F. Valle

We consider the generation of the hierarchical charged lepton spectrum and anarchic neutrino masses and mixing angles in warped extra dimensional models with Randall-Sundrum metric. We have classified all possible cases giving rise to…

高能物理 - 唯象学 · 物理学 2015-06-11 Gero von Gersdorff , Mariano Quiros , Michael Wiechers

It has recently been shown that the neutrino can have non-zero electric charge in a number of gauge theories, including the Minimal Standard Model. Assuming non-zero neutrino charge, we develop a new approach to the solar neutrino problem.…

高能物理 - 唯象学 · 物理学 2011-07-19 A. Yu. Ignatiev , G. C. Joshi

The difference between baryon number B and lepton number L is the only anomaly-free global symmetry of the Standard Model, easily promoted to a local symmetry by introducing three right-handed neutrinos, which automatically make neutrinos…

高能物理 - 唯象学 · 物理学 2014-11-11 Julian Heeck

Majorana features of neutrinos and SO(3) gauge symmetry of three families enable us to construct a gauge model of neutrino for understanding naturally the observed smallness of neutrino masses and the nearly tri-bimaximal neutrino mixing…

高能物理 - 唯象学 · 物理学 2012-03-06 Yue-Liang Wu

The MiniBooNE low-energy excess stands as an unexplained anomaly in short-baseline neutrino oscillation experiments. It has been shown that it can be explained in the context of dark sector models. Here, we provide an overview of the…

高能物理 - 唯象学 · 物理学 2025-01-31 Asli M. Abdullahi , Jaime Hoefken Zink , Matheus Hostert , Daniele Massaro , Silvia Pascoli

Little Higgs models are formulated as effective theories with a cut-off of up to 100 times the electroweak scale. Neutrino masses are then a puzzle, since the usual see-saw mechanism involves a much higher scale that would introduce…

高能物理 - 唯象学 · 物理学 2009-11-11 F. del Aguila , M. Masip , J. L. Padilla

A new era in particle physics is being spurred on by new data from the Large Hadron Collider. Non-vanishing neutrino masses represent firm observational evidence of new physics beyond the Standard Model. An extension of the latter, based on…

高能物理 - 唯象学 · 物理学 2015-06-05 S. Khalil , S. Moretti

The observed deficit of $\rm ^8B$ solar neutrinos may call for an improved standard model of the sun or an expanded standard model of particle physics ({\it e.g.,} with neutrino masses and mixing). In the former case, contemporary fluid…

高能物理 - 唯象学 · 物理学 2007-05-23 A. De Rújula , S. L. Glashow

We discuss an extended SU(2)XU(1) model which naturally leads to mass scales and mixing angles relevant for understanding both the solar and atmospheric neutrino anomalies in terms of the vacuum oscillations of the three known neutrinos.…

高能物理 - 唯象学 · 物理学 2010-04-06 Anjan S. Joshipura , Saurabh D. Rindani

We present a relationship, E_\nu^{max} = m_{\nu} M_{Planck}/M_{weak}, among the highest observed neutrino energy (~PeV) and the neutrino mass, the weak scale, and the Planck energy. We then discuss some tests of this relationship, and…

高能天体物理现象 · 物理学 2014-07-04 John G. Learned , Thomas J. Weiler

Neutrinos are amongst the most abundant particles in the universe. The fact that they are massive particles proves that the Standard Model is an incomplete theory and needs to be extended. This thesis focuses on the study of neutrino…

高能物理 - 唯象学 · 物理学 2023-09-28 Pablo Martínez-Miravé

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

Neutrino oscillations data indicates that neutrino mixings are consistent with an apparent $\nu_\mu - \nu_\tau$ exchange symmetry in neutrino mass matrix. We observe that in the mininimally extended standard model with the see-saw…

高能物理 - 唯象学 · 物理学 2008-11-26 Juan Carlos Gómez-Izquierdo , Abdel Pérez-Lorenzana

We consider supersymmetric models where the scale of supersymmetry breaking lies between 5 $\times 10^6$ GeV and 5 $\times 10^8$ GeV. In this class of theories, which includes models of gauge mediated supersymmetry breaking, the lightest…

高能物理 - 唯象学 · 物理学 2009-11-10 I. Albuquerque , G. Burdman , Z. Chacko

Observational evidences of nonzero neutrino masses and the existence of dark matter request physics beyond standard model. A model with extra scalars and leptonic vector-like fermions is introduced. By imposing a Z_2 symmetry, the neutrino…

高能物理 - 唯象学 · 物理学 2011-04-20 Chian-Shu Chen , Chung-Hsien Chou

We can start with the question: why are neutrino properties especially interesting? Recall that in the minimal standard model there are no right handed neutrinos and furthermore lepton number is conserved so neutrinos can have neither Dirac…

高能物理 - 唯象学 · 物理学 2007-05-23 S. Pakvasa