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A two-parameter neutrino mass formula is described, giving a moderately hierarchical spectrum m_1 < m_2 < m_3 consistent with the experimental estimates of Delta m^2_{21} and Delta m^2_{32}. The formula follows from a three-parameter…

综合物理 · 物理学 2007-06-20 Wojciech Krolikowski

Deviations from expectations have been claimed for solar, atmospheric and high energy prompt neutrinos from charm decay. This information, supplemented only by the existing very good upper limits for oscillations of the $\nu_{\mu}$ at…

高能物理 - 唯象学 · 物理学 2011-05-23 G. Conforto , A. Marchionni , F. Martelli , F. Vetrano , M. Lanfranchi , G. Torricelli-Ciamponi

An elegant model is proposed by extending the Standard Model using the $\Delta(27)\times Z_3 \times Z_{10}$ symmetry within the framework of the Type-I + Type-II seesaw mechanism. This model is particularly noteworthy for its ability to…

高能物理 - 唯象学 · 物理学 2025-03-26 Manash Dey , Subhankar Roy

Seesaw mechanisms are the simplest and the most elegant way of generating small masses for the active neutrinos $(m_\nu)$. In these mechanisms $m_\nu$ is inversely proportional to the lepton number breaking scale $(M)$ that, in the…

高能物理 - 唯象学 · 物理学 2023-05-01 E. Cabrera , D. Cogollo , C. A. de S. Pires

Even if quark and lepton masses are not uniquely predicted by the fundamental theory, as may be the case in the string theory landscape, nevertheless their pattern may reveal features of the underlying theory. We use statistical techniques…

高能物理 - 唯象学 · 物理学 2014-11-18 John F. Donoghue , Koushik Dutta , Andreas Ross

Using the seesaw mechanism and a discrete symmetry, we construct a class of models for the neutrino mass matrix where the inverse of that matrix is the sum of a mu-tau antisymmetric background and a perturbation. We consider various…

高能物理 - 唯象学 · 物理学 2009-11-11 Walter Grimus , Satoru Kaneko , Luis Lavoura , Hideyuki Sawanaka , Morimitsu Tanimoto

We show that the addition of real scalars (gauge singlets) to the Standard Model can both ameliorate the little hierarchy problem and provide realistic Dark Matter candidates. To this end, the coupling of the new scalars to the standard…

高能物理 - 唯象学 · 物理学 2010-04-23 Bohdan Grzadkowski , Jose Wudka

Possibility of a Right-Handed (RH) neutrino being a Goldstone fermion of a spontaneously broken global $U(1)$ symmetry in a supersymmetric theory is considered. This fermion obtains mass from the supergravity effects leading to a RH…

高能物理 - 唯象学 · 物理学 2021-10-08 Anjan S. Joshipura , Ketan M. Patel

We consider a class of models in which the neutrinos acquire Majorana masses through mixing with singlet neutrinos that emerge as composite states of a strongly coupled hidden sector. In this framework, the light neutrinos are partially…

高能物理 - 唯象学 · 物理学 2021-03-16 Zackaria Chacko , Patrick J. Fox , Roni Harnik , Zhen Liu

We propose models for neutrino masses and mixing in the framework of low scale $U(1)_{L_\mu-L_\tau}$ gauge extension of the standard model. The models are designed to spontaneously break $U(1)_{L_\mu-L_\tau}$ so that the…

高能物理 - 唯象学 · 物理学 2019-11-20 Takeshi Araki , Kento Asai , Joe Sato , Takashi Shimomura

A new idea for neutrino mass was proposed recently, where its smallness is not due to the seesaw mechanism, i.e. not inversely proportional to some large mass scale. It comes from a one-loop mechanism with dark matter in the loop consisting…

高能物理 - 唯象学 · 物理学 2013-06-06 Subhaditya Bhattacharya , Ernest Ma , Alexander Natale , Ahmed Rashed

Mixing between light and heavy neutrino states has been proposed as an explanation (or partial explanation) for the 3-sigma NuTeV anomaly and the 2-sigma departure of the $Z^0$ invisible width from its expected value. I assume herein that…

高能物理 - 唯象学 · 物理学 2016-09-06 Sheldon Lee Glashow

The Neutrino Option is a scenario where the Higgs mass is generated at the same time as neutrino masses in the type-I seesaw model. This framework provides a dynamical origin for the scalar potential of the Standard Model and suggests a new…

高能物理 - 唯象学 · 物理学 2019-04-30 Ilaria Brivio

We determine the nu_{R} Majorana mass matrix from the experimental data on neutrino oscillations in the framework of a see-saw SO(10) model, where we impose the condition (M^R)_{33} = 0 to avoid too large fine-tunings in the see-saw…

高能物理 - 唯象学 · 物理学 2015-06-25 M. Abud , F. Buccella

An extension of the Standard Model (SM) is studied in which two right-handed (RH) neutrinos per generation are incorporated, but considering the hypothesis of the symmetry of lepton and quark contents in order to deprive the number of RH…

高能物理 - 唯象学 · 物理学 2015-01-13 Ernesto A. Matute

We studied a left-right symmetric model that can accommodate the neutrino dark energy (\nd) proposal. Type III seesaw mechanism is implemented to give masses to the neutrinos. After explaining the model, we study the consistency of the…

高能物理 - 唯象学 · 物理学 2010-04-21 Jitesh R. Bhatt , Pei-Hong Gu , Utpal Sarkar , Santosh K. Singh

We study the consequences of the $Z_2$-symmetry behind the $\mu$--$\tau$ universality in neutrino mass matrix. We then implement this symmetry in the type-I seesaw mechanism and show how it can accommodate all sorts of lepton mass…

高能物理 - 唯象学 · 物理学 2015-07-01 E. I. Lashin , N. Chamoun , C. Hamzaoui , S. Nasri

If neutrinos have masses, why are they so tiny? Are these masses of the Dirac type or of the Majorana type? We are already familiar with the mechanism of how to obtain a tiny Majorana neutrino mass by the famous see-saw mechanism. The…

高能物理 - 唯象学 · 物理学 2009-10-31 P. Q. Hung

We discuss a simple theory for neutrino masses where the total lepton number is a local gauge symmetry spontaneously broken below the multi-TeV scale. In this context, the neutrino masses are generated through the canonical seesaw mechanism…

高能物理 - 唯象学 · 物理学 2024-07-02 Hridoy Debnath , Pavel Fileviez Perez , Kevin Gonzalez-Quesada

Using the family symmetry, in the neutrino mass matrix we remove the Yukawa coupling (arising in the Dirac type mass between the heavy neutrinos and light lepton doublets) dependence in the double seesaw mechanism so that it is directly…

高能物理 - 唯象学 · 物理学 2009-11-11 Jihn E. Kim , Jong-Chul Park
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