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We propose a minimal predictive inverse seesaw model based on two right-handed neutrinos and two additional singlets, leading to the same low energy neutrino mass matrix as in the Littlest Seesaw (LS) (type I) model. In order to implement…

高能物理 - 唯象学 · 物理学 2020-03-02 A. E. Cárcamo Hernández , S. F. King

We study the minimal seesaw model, where two right-handed Majorana neutrinos are introduced, focusing on the CP violating phase. In addition, we take the trimaximal mixing pattern for the neutrino flavor where the charged lepton mass matrix…

高能物理 - 唯象学 · 物理学 2018-01-17 Yusuke Shimizu , Kenta Takagi , Morimitsu Tanimoto

The compatibility of the Frobenius group T13 with the canonical see-saw mechanism of neutrino mixing is examined. The Standard Model is extended in a minimalist way, by introducing a family symmetry and three right-handed neutrinos. To fit…

高能物理 - 唯象学 · 物理学 2013-05-30 Christine Hartmann

In this paper, we have realized the left-right symmetric model with modular symmetry. We have used $\Gamma$(3) modular group which is isomorphic to non-abelian discrete symmetry group $A_4$. The advantage of using modular symmetry is the…

高能物理 - 唯象学 · 物理学 2023-02-01 Ankita Kakoti , Bichitra Bijay Boruah , Mrinal Kumar Das

We investigate the renormalization group evolution of masses and mixing angles of Majorana neutrinos under the `High Scale Mixing Unification' hypothesis. Assuming the unification of quark-lepton mixing angles at a high scale, we show that…

高能物理 - 唯象学 · 物理学 2014-05-23 Gauhar Abbas , Saurabh Gupta , G. Rajasekaran , Rahul Srivastava

We considered a model where |V_{13}|=0 so that delta=0 at M_R and analyzed mixing angles and CP violation angles at the low energy scale by using the renormalization group in the MSSM model. In this model, parameters at M_R scale are two…

高能物理 - 唯象学 · 物理学 2015-06-25 Takahiro Miura , Tetsuo Shindou , Eiichi Takasugi

The simplest unified extension of the Minimal Supersymmetric Standard Model with bi-linear R--Parity violation provides a predictive scheme for neutrino masses which can account for the observed atmospheric and solar neutrino anomalies in…

高能物理 - 唯象学 · 物理学 2008-11-26 J. C. Romao , M. A. Diaz , M. Hirsch , W. Porod , J. W. F Valle

We systematically analyze the radiative corrections to the $S_3$ symmetric neutrino mass matrix at high energy scale, say the GUT scale, in the charged lepton basis. There are significant corrections to the neutrino parameters both in the…

高能物理 - 唯象学 · 物理学 2015-06-22 Shivani Gupta , C. S. Kim , Pankaj Sharma

The $\mu \nu$SSM proposes to use right-handed neutrino supermultiplets in order to generate the $\mu$ term and neutrino masses simultaneously. We discuss neutrino physics and the associated electroweak seesaw mechanism in this model. We…

高能物理 - 唯象学 · 物理学 2010-04-07 Daniel E. Lopez-Fogliani

The smallness of the neutrino masses can be well understood within the seesaw mechanism. We analyse two cases of the minimal extension of the standard model when one or two right-handed fields are added to the three left-handed fields. A…

高能物理 - 唯象学 · 物理学 2014-12-19 Darius Jurciukonis , Thomas Gajdosik , Andrius Juodagalvis , Tomas Sabonis

There are several indications that the Majorana masses of the right-handed neutrino components, $M_R,$ are at the intermediate scale: $M_R\sim (10^{10}-10^{12})$ GeV or even lighter. The renormalization effects due to large Yukawa couplings…

高能物理 - 唯象学 · 物理学 2009-10-28 F. Vissani , A. Yu. Smirnov

In this paper, we construct a model with the help of modular symmetry in the framework of minimal inverse seesaw [ISS(2,3)]. We have used $\Gamma(3)$ modular group which is isomorphic to non-Abelian discrete symmetry group $A_4$. In this…

高能物理 - 唯象学 · 物理学 2023-05-03 Jotin Gogoi , Nayana Gautam , Mrinal Kumar Das

If the scale dependence of a Yukawa matrix is assumed to be determined entirely by the dominant 33-element, then the renormalization group equations can be expressed in terms of two separate equations: a differential equation for the…

高能物理 - 唯象学 · 物理学 2007-05-23 Bipin R. Desai , Alexander R. Vaucher

In light of the recent solar and atmospheric neutrino data, we investigate the possibility of having an exactly degenerate spectrum for heavy right-handed Majorana neutrinos at the grand unification scale. The analysis is performed in the…

高能物理 - 唯象学 · 物理学 2010-02-03 R. Gonzalez Felipe , F. R. Joaquim

We analyse a supersymmetric string-inspired model of all fermion masses and mixing angles based on the Pati-Salam $SU(4)\times SU(2)_L \times SU(2)_R$ gauge group supplemented by a $U(1)_X$ flavour symmetry. The model involves third family…

高能物理 - 唯象学 · 物理学 2016-09-06 S. F. King , M. Oliveira

Low energy effects induced by heavy extra degrees of freedom are suppressed by powers of the large mass scale, thus preserving, if sufficiently heavy, the successes of the Standard Model in describing low energy phenomena. However, as is…

高能物理 - 唯象学 · 物理学 2015-05-28 Alejandro Ibarra , Cristoforo Simonetto

We study renormalization group running effects on neutrino mixing patterns when a (type I) seesaw model is implemented by suitable flavour symmetries. We are particularly interested in mass-independent mixing patterns to which the widely…

高能物理 - 唯象学 · 物理学 2010-05-28 Yin Lin , Luca Merlo , Alessio Paris

This is a review article about neutrino mass models, particularly see-saw models involving three active neutrinos which are capable of describing both the atmospheric neutrino oscillation data, and the large mixing angle MSW solar solution,…

高能物理 - 唯象学 · 物理学 2009-11-10 S. F. King

We consider the problem of neutrino masses and mixing within the general framework of standard (type-I) seesaw models leading to three light neutrinos. Under the assumption of a hierarchical neutrino mass spectrum \lambda^4: \lambda : 1,…

高能物理 - 唯象学 · 物理学 2013-05-30 M. Paraskevas , K. Tamvakis

We consider the simplest model which solves the solar and atmospheric neutrino puzzles, in the sense that it contains the smallest amount of beyond the Standard Model ingredients. The solar neutrino data is accounted for by Planck-mass…

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