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We propose a new neutrino flavor model based on a $D_{4}\times U(1)$ flavor symmetry providing predictions for neutrino masses and mixing along with a successful generation of the observed Baryon Asymmetry of the Universe (BAU). After the…

高能物理 - 唯象学 · 物理学 2024-04-26 M. Miskaoui

We propose a model with $D_4$ flavor symmetry for leptogenesis in the framework of supersymmetric $SU(5)$ grand unified theory. Neutrino masses arise from the type I seesaw mechanism where the spontaneous symmetry breaking of the flavor…

高能物理 - 唯象学 · 物理学 2022-06-06 M. A. Loualidi , M. Miskaoui

We present a simple extension of the Standard Model with three right-handed neutrinos in a SUSY framework, with an additional U(1$)_\text{F}$ abelian flavor symmetry with a non standard leptonic charge $L_e-L_\mu-L_\tau$ for lepton doublets…

高能物理 - 唯象学 · 物理学 2023-03-01 Giorgio Arcadi , Simone Marciano , Davide Meloni

We study baryogenesis via leptogenesis in an extension of the Standard Model by adding one right-handed neutrino and one triplet scalar. These heavy particles contribute to the generation of tiny neutrino mass through seesaw mechanism. The…

高能物理 - 唯象学 · 物理学 2023-06-28 Sreerupa Chongdar , Sasmita Mishra

We study $S_{4}$ flavor symmetric inverse seesaw model which has the possibility of simultaneously addressing neutrino phenomenology, dark matter (DM) and baryon asymmetry of the universe (BAU) through leptogenesis. The model is the…

高能物理 - 唯象学 · 物理学 2021-09-01 Nayana Gautam , Mrinal Kumar Das

We present an S$_4$ flavour symmetric model within a minimal seesaw framework resulting in mass matrices that leads to TM$_1$ mixing. Minimal seesaw is realized by adding two right-handed neutrinos to the Standard Model. The model predicts…

高能物理 - 唯象学 · 物理学 2021-12-22 Bikash Thapa , Ng. K. Francis

The possibility to explain the baryon asymmetry in the Universe through the leptogenesis mechanism in the context of Adjoint SU(5) is investigated. In this model the neutrino masses are generated through the Type I and Type III seesaw…

高能物理 - 唯象学 · 物理学 2008-11-26 Steve Blanchet , Pavel Fileviez Perez

We propose a minimal $A_4$ flavor symmetric model, assisted by $Z_2 \times Z_3$ symmetry, which can naturally takes care of the appropriate lepton mixing and neutrino masses via Type-I seesaw. It turns out that the framework, originated due…

高能物理 - 唯象学 · 物理学 2022-01-05 Arghyajit Datta , Biswajit Karmakar , Arunansu Sil

Extending the Standard Model with right-handed neutrinos provides a minimal explanation for both light neutrino masses (through the type-I seesaw mechanism) and the baryon asymmetry of our universe (through leptogenesis). We map here for…

高能物理 - 唯象学 · 物理学 2023-05-12 Yannis Georis

We study the possibility of generating non-zero reactor mixing angle $\theta_{13}$ and baryon asymmetry of the Universe within the framework of an $A_4$ flavour symmetric model. Using the conventional type I seesaw mechanism we construct…

高能物理 - 唯象学 · 物理学 2018-06-13 Debasish Borah , Mrinal Kumar Das , Ananya Mukherjee

We investigate baryogenesis via leptogenesis in $A_4$ flavor model within the paradigm of type-I and II seesaw mechanism resulting in magic neutrino mass matrix with broken $\mu-\tau$ symmetry in a minimal scenario with two right-handed…

高能物理 - 唯象学 · 物理学 2020-08-26 Surender Verma , Monal Kashav

We compute and compare the baryon asymmetry of the universe in thermal leptogenesis scenario with and without flavour effects for different neutrino mass models namely degenerate, inverted hierarchical and normal hierarchical models, with…

高能物理 - 唯象学 · 物理学 2009-11-13 H. Zeen Devi , Amal Kr Sarma , N. Nimai Singh

The baryon to photon ratio in the present Universe is very accurately measured to be $(6.065 \pm 0.090) \times 10^{-10}$. We study the possible origin of this baryon asymmetry in the neutrino sector through the generic mechanism of…

高能物理 - 唯象学 · 物理学 2014-07-10 Debasish Borah , Mrinal Kumar Das

We consider a model with three right-handed neutrinos in which Yukawa coupling constants and Majorana masses are obtained by requiring the modular $A_4$ symmetry. It has been shown that the model can explain mass hierarchies and mixing…

高能物理 - 唯象学 · 物理学 2021-06-01 Takehiko Asaka , Yongtae Heo , Takuya H. Tatsuishi , Takahiro Yoshida

In this paper, we would like to point out that in the scenario that the right-handed neutrinos suddenly gain some masses much larger than the temperature of the Universe at that time so that the washout effects for the lepton asymmetry…

高能物理 - 唯象学 · 物理学 2024-09-18 Zhen-hua Zhao , Jing Zhang , Xiang-Yi Wu

The generation of the right amount of baryon asymmetry $\eta$ of the Universe from supersymmetric leptogenesis is studied within the type-I seesaw framework with three heavy singlet Majorana neutrinos $N_i\,\,(i = 1,2,3)$ and their…

高能物理 - 唯象学 · 物理学 2011-01-28 Biswajit Adhikary , Ambar Ghosal , Probir Roy

The extension of the Standard Model by heavy right-handed neutrinos can simultaneously explain the observed neutrino masses via the seesaw mechanism and the baryon asymmetry of the Universe via leptogenesis. If the mass of the heavy…

高能物理 - 唯象学 · 物理学 2020-07-10 Marco Drewes , Bjorn Garbrecht , Dario Gueter , Juraj Klaric

We investigate the relation between non-unitarity of the leptonic mixing matrix and leptogenesis. We discuss how all parameters of the canonical type-I seesaw mechanism can, in principle, be reconstructed from the neutrino mass matrix and…

高能物理 - 唯象学 · 物理学 2011-05-23 Stefan Antusch , Steve Blanchet , Mattias Blennow , Enrique Fernandez-Martinez

Baryogenesis via leptogenesis is investigated in a specific model of light neutrino masses and mixing angles. The latter was proposed on the basis of an assumed complex-extended scaling property of the neutrino Majorana mass matrix $M_\nu$,…

高能物理 - 唯象学 · 物理学 2017-03-22 Rome Samanta , Mainak Chakraborty , Probir Roy , Ambar Ghosal

In this paper, we investigate leptogenesis under the neutrino mass anarchy hypothesis in both type-I and type-II seesaw models. We first revisit the corresponding study in the type-I seesaw framework with two improvements: in contrast to…

高能物理 - 唯象学 · 物理学 2026-03-31 Qi An , Yan Shao , Zhen-hua Zhao
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