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With a mass at least six orders of magnitudes smaller than the mass of an electron -- but non-zero -- neutrinos are a clear misfit in the Standard Model of Particle Physics. On the one hand, its tiny mass makes the neutrino one of the most…

核实验 · 物理学 2016-06-22 Susanne Mertens

Considering a general mass matrix for quasi-degenerate neutrinos and treating the experimentally known oscillation parameters as inputs, we study the correlation between the degenerate mass scale $(m)$ and the mixing angle $\theta_{13}$. We…

高能物理 - 唯象学 · 物理学 2008-11-26 Rathin Adhikari , Anindya Datta , Biswarup Mukhopadhyaya

We revisit the possibility of generating non-zero reactor mixing angle in a scenario where there is a sterile neutrino at the eV scale apart from the usual three sub-eV scale active neutrinos. We show that the $3\times3$ active neutrino…

高能物理 - 唯象学 · 物理学 2017-02-22 Debasish Borah

In spite of enormous experimental progress in determination of the neutrino parameters, theory of neutrino mass and mixing is still on the cross-roads. Guidelines could be (i) the connection between zero neutrino charges (and therefore a…

高能物理 - 唯象学 · 物理学 2022-03-02 Alexei Yu. Smirnov

We find a realization of the $Z_2$-symmetry in the neutrino mass matrix which expresses a rotation of the $\mu-\tau$ symmetry and is able to impose a generic smallest mixing angle, in contrast to a zero-value predicted by the usual…

高能物理 - 唯象学 · 物理学 2017-07-12 E. I. Lashin , N. Chamoun , C. Hamzaoui , S. Nasri

Is the relatively isolated member of the neutrino mass spectrum heavier or lighter than the two closely-spaced members? This question - the character of the neutrino mass hierarchy - is of great theoretical interest. All previously…

高能物理 - 唯象学 · 物理学 2008-11-26 Andre de Gouvea , James Jenkins , Boris Kayser

A generalized phenomenological (3 + 2 + 1)-model with three active and three sterile neutrinos is considered for the calculation of the neutrino oscillation characteristics at normal mass hierarchy of active neutrinos and significant…

高能物理 - 唯象学 · 物理学 2016-12-28 V. V. Khruschov , S. V. Fomichev , O. A. Titov

A brief review of the experimental status of neutrino mixing. The model of neutrino oscillations has now been established with high confidence, with many of the model parameters measured to an accuracy of a few per cent. However, some…

高能物理 - 实验 · 物理学 2011-07-21 Justin Evans

A class of neutrino mass matrices with texture zeros realizable using the group $Z_3$ within the framework of type (I+II) seesaw mechanism naturally admits a non-zero $\theta_{13}$ and allows for deviations from maximal mixing. The…

高能物理 - 唯象学 · 物理学 2015-05-30 Sanjeev Kumar

We review the current status of the neutrino mass and mixing parameters needed to reconstruct the neutrino mass matrix. A comparative study of the precision in the measurement of oscillation parameters expected from the next generation…

高能物理 - 唯象学 · 物理学 2016-09-06 Sandhya Choubey

We consider the running of the neutrino mass matrix in the Standard Model and the Minimal Supersymmetric Standard Model, extended by heavy singlet Majorana neutrinos. Unlike previous studies, we do not assume that all of the heavy mass…

高能物理 - 唯象学 · 物理学 2015-06-25 Stefan Antusch , Joern Kersten , Manfred Lindner , Michael Ratz

Restrictions on the neutrino masses and lepton mixing are reviewed. Solar, atmospheric and relic neutrinos give the indications of existence of nonzero neutrino masses and mixing. The data pick up two regions of mixing angles which are or…

高能物理 - 唯象学 · 物理学 2009-09-25 Alexei Yu. Smirnov

We review in this talk various SUSY SO(10) models. Specifically, we discuss how small neutrino masses are generated in and generic predictions of different SO(10) models. A comparison of the predictions of these models for…

高能物理 - 唯象学 · 物理学 2009-11-10 Mu-Chun Chen , K. T. Mahanthappa

In 2004, two of us proposed a texture, the "Simplest" neutrino mass matrix, which predicted sin(theta13)=sqrt((2 Solar-Delta m^2)/(3 Atm-Delta m^2)) and delta_CP=90 degrees. Using today's measured values for neutrino mass-squared…

高能物理 - 唯象学 · 物理学 2013-07-31 R. Krishnan , P. F. Harrison , W. G. Scott

Neutrinos are neutral, spin-$\frac{1}{2}$ particles which undergo only weak interactions. The experimentally observed phenomenon of neutrino oscillation establishes the fact that neutrinos are massive and there is mixing between different…

高能物理 - 唯象学 · 物理学 2016-03-16 Monojit Ghosh

A new and radical scenario of the simple 2006 model of radiative neutrino mass is proposed, where there is no seesaw mechanism, i.e. neutrino masses are not inversely proportional to some large mass scale, contrary to the prevalent…

高能物理 - 唯象学 · 物理学 2015-06-05 Ernest Ma

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

Radiative generation of realistic mixing in neutrino sector is studied at one-loop level in a scotogenic $A4\times Z_2$ symmetric framework. A scheme of obtaining non-zero $\theta_{13}$ through small mass splitting in right-handed neutrino…

高能物理 - 唯象学 · 物理学 2019-03-12 Soumita Pramanick

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…

高能物理 - 唯象学 · 物理学 2010-09-14 Fu-Sin Ling

A minimal extension of the standard model to naturally generate small neutrino masses and provide a dark matter candidate is proposed. The dark matter particle is part of a new scalar doublet field that plays a crucial role in radiatively…

高能物理 - 唯象学 · 物理学 2014-07-03 Michael Gustafsson , Jose Miguel No , Maximiliano A. Rivera