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相关论文: Simplest Scoto-Seesaw Mechanism

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We propose a novel and minimal framework where a light scalar field can give rise to dark matter (DM) self-interactions, while enhancing the CP symmetry required for successful baryon asymmetry of the Universe via leptogenesis route. For…

高能物理 - 唯象学 · 物理学 2022-12-07 Debasish Borah , Arnab Dasgupta , Satyabrata Mahapatra , Narendra Sahu

The seesaw model of neutrinos might explain the size, age, flatness and near-homogeneity of the Universe via sneutrino inflation, as well as explaining the origin of matter via leptogenesis. The sneutrino inflation hypothesis makes…

高能物理 - 唯象学 · 物理学 2008-11-26 John Ellis

In the framework of the seesaw mechanism with three heavy right-handed Majorana neutrinos and no Higgs triplets we carry out a systematic study of the structure of the right-handed neutrino sector. Using the current low-energy neutrino data…

高能物理 - 唯象学 · 物理学 2009-11-10 Evgeny Kh. Akhmedov , Michele Frigerio , Alexei Yu. Smirnov

We extend the singlet Majoron model of dark radiation by adding another singlet scalar of unit lepton charge. The spontaneous breaking of global $U(1)_L$ connects dark radiation with neutrino mass generation via the type-I seesaw mechanism.…

高能物理 - 唯象学 · 物理学 2014-10-08 We-Fu Chang , John N. Ng

Specific class of textures for the Dirac and Majorana mass matrices in the seesaw model leading to a pair of almost degenerate neutrinos is discussed. These textures can be obtained by imposing a horizontal $U(1)$ symmetry. A specific model…

高能物理 - 唯象学 · 物理学 2009-10-28 Gautam Dutta , Anjan S. Joshipura

Cosmological constraints on the sum of the neutrino masses can be relaxed if the number density of active neutrinos is reduced compared to the standard scenario, while at the same time keeping the effective number of neutrino species…

高能物理 - 唯象学 · 物理学 2024-06-24 Miguel Escudero , Thomas Schwetz , Jorge Terol-Calvo

We develop a recipe which allows one to recursively and uniquely decouple the large scale from the small scale in mass matrices of the seesaw type, up to any order in the inverse of the large scale. Our method allows one to calculate the…

高能物理 - 唯象学 · 物理学 2009-10-31 W. Grimus , L. Lavoura

The seesaw mechanism is the most attractive mechanism to explain the small neutrino masses, which predicts the neutrinoless double beta decay ($0\nu\beta\beta$) of the nucleus. Thus the discovery of $0\nu\beta\beta$ is extremely important…

高能物理 - 唯象学 · 物理学 2023-12-19 Yu-Cheng Qiu , Jin-Wei Wang , Tsutomu T. Yanagida

The usual see-saw formula is modified by the presence of two Higgs triplets in left-right symmetric theories. The contribution from the left-handed Higgs triplet to the see-saw formula can dominate over the conventional one when the…

高能物理 - 唯象学 · 物理学 2010-02-03 A. S. Joshipura , E. A. Paschos , W. Rodejohann

We suggest that quintessential vacuum energy could be the source of right handed neutrino masses that feed the seesaw mechanism, which may provide observed small masses to light standard neutrinos. This idea is naturally implemented in the…

高能物理 - 唯象学 · 物理学 2020-04-22 J. G. Salazar-Arias , Abdel Pérez-Lorenzana

The see-saw mechanism for neutrino masses based on the Grand Unification leads to the mass of the heaviest neutrino ($\approx \nu_{\tau}$) in the range $(2 - 3)\cdot 10^{-3}$ eV and hence to a solution of the solar neutrino problem through…

高能物理 - 唯象学 · 物理学 2011-07-19 Anjan S. Joshipura , A. Yu. Smirnov

A simple 3 X 3 neutrino mass matrix is proposed to accommodate both the solar and atmospheric neutrino deficits. This scenario can be realized naturally by a radiative mechanism for the generation of neutrino masses. It also goes together…

高能物理 - 唯象学 · 物理学 2010-01-06 Ernest Ma

In the framework of SO(10) gauge unification and the seesaw mechanism, we show that the upper bound on the mass of the heaviest right-handed neutrino $M_{R_3} < 3 \times 10^{11}$ GeV, given by the Pati-Salam intermediate scale of $B-L$…

高能物理 - 唯象学 · 物理学 2015-05-28 M. Abud , F. Buccella , D. Falcone , L. Oliver

In the framework of type II seesaw mechanism we propose two simple but instructive ansatze for neutrino mixing and leptogenesis. In each ansatz, the effective Majorana neutrino mass matrix is composed of two parts -- the part with Z_2…

高能物理 - 唯象学 · 物理学 2008-11-26 Wan-lei Guo

An alternative to the famous see-saw mechanism is proposed to explain the smallness of the neutrino masses (if present). This model involves a fourth family which mixes very little with the other three. It contains one heavy neutrino (mN >…

高能物理 - 唯象学 · 物理学 2007-05-23 P. Q. Hung

We investigate an extension of the Minimal Standard Model by right-handed neutrinos (the $\nu$MSM) to incorporate neutrino masses consistent with oscillation experiments. Within this theory, the only candidates for dark matter particles are…

高能物理 - 唯象学 · 物理学 2008-11-26 Takehiko Asaka , Steve Blanchet , Mikhail Shaposhnikov

We study sterile neutrino dark matter in a minimal Type-I Dirac seesaw framework where the states responsible for generating Dirac neutrino masses at tree level can be viable dark matter candidates. A $\mathcal{Z}_6$ symmetry, spontaneously…

高能物理 - 唯象学 · 物理学 2026-03-23 J. Adhikary , A. Batra , K. Deka , F. R. Joaquim

We propose a left-right symmetric electroweak extension of the Standard Model based on the $\Delta \left( 27\right)$ family symmetry. The masses of all electrically charged Standard Model fermions lighter than the top quark are induced by a…

高能物理 - 唯象学 · 物理学 2019-05-14 A. E. Cárcamo Hernández , Sergey Kovalenko , José W. F. Valle , C. A. Vaquera-Araujo

We propose a minimal model where a dark sector, odd under a $\mathcal{Z}_2$ discrete symmetry, is the seed of lepton number violation in the neutrino sector at the loop level, in the context of the linear seesaw mechanism. Neutrino mass…

高能物理 - 唯象学 · 物理学 2023-07-19 A. Batra , H. B. Câmara , F. R. Joaquim

Neutrino data lead via the see-saw mechanism to masses of the right handed neutrinos at the intermediate mass scale. Simple formalism is suggested which incorporates the quark - lepton symmetry and allows one to find properties of the…

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