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相关论文: On the Minimal Mixing of Heavy Neutrinos

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We consider the Standard Model extended by right-handed neutrinos to explain massive neutrinos through the seesaw mechanism. The new fermion can be observed when it has a sufficiently small mass and large mixings to left-handed neutrinos.…

高能物理 - 唯象学 · 物理学 2015-12-17 Takehiko Asaka , Takanao Tsuyuki

In the type-I seesaw model the size of mixing between light and heavy neutrinos, nu and N, respectively, is of order the square root of their mass ratio, (m_nu/m_N)^(1/2), with only one generation of the neutrinos. Since the light-neutrino…

高能物理 - 唯象学 · 物理学 2010-06-21 Xiao-Gang He , Sechul Oh , Jusak Tandean , Chung-Cheng Wen

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

The existence of the tiny neutrino mass and the flavor mixing can be naturally explained by type-I Seesaw model which is probably the simplest extension of the Standard Model (SM) using Majorana type SM gauge singlet heavy Right Handed…

高能物理 - 唯象学 · 物理学 2018-04-25 Arindam Das

We consider the minimal seesaw model, the Standard Model extended by two right-handed neutrinos, for explaining the neutrino masses and mixing angles measured in oscillation experiments. When one of right-handed neutrinos is lighter than…

高能物理 - 唯象学 · 物理学 2023-07-26 Takehiko Asaka , Hiroyuki Ishida , Kazuki Tanaka

The neutrino masses and flavor mixings, which are missing in the Standard Model (SM), can be naturally incorporated in the type-I seesaw extension of the SM with heavy Majorana neutrinos being singlet under the SM gauge group. If the heavy…

高能物理 - 唯象学 · 物理学 2018-03-21 Arindam Das , Nobuchika Okada

We consider an extension of the Standard Model with three right-handed (RH) neutrinos and a Dirac pair of extra sterile neutrinos, odd under a discrete $Z_2$ symmetry, in order to have left-right symmetry in the neutrino content and obtain…

高能物理 - 唯象学 · 物理学 2021-08-11 Ernesto A. Matute

We consider the seesaw mechanism of neutrino mass generation in the light of our present knowledge of the neutrino masses and mixing. We analyse the seesaw mechanism constrained by the following assumptions: (1) minimal seesaw with no Higgs…

高能物理 - 唯象学 · 物理学 2008-11-26 E. Kh. Akhmedov , G. C. Branco , M. N. Rebelo

We consider seesaw type-I models including at least one (mostly-)sterile neutrino with mass at the eV scale. Three distinct situations are found, where the presence of light extra neutrinos is naturally justified by an approximately…

高能物理 - 唯象学 · 物理学 2020-08-26 G. C. Branco , J. T. Penedo , Pedro M. F. Pereira , M. N. Rebelo , J. I. Silva-Marcos

In the type-I seesaw mechanism, both the light Majorana neutrinos (\nu_1, \nu_2, \nu_3) and the heavy Majorana neutrinos (N_1, ..., N_n) can mediate the neutrinoless double-beta (0\nu\beta\beta) decay. We point out that the contribution of…

高能物理 - 唯象学 · 物理学 2009-09-28 Zhi-zhong Xing

We consider theories where the Standard Model (SM) neutrinos acquire masses through the seesaw mechanism at the weak scale. We show that in such a scenario, the requirement that any pre-existing baryon asymmetry, regardless of its origin,…

高能物理 - 唯象学 · 物理学 2010-04-14 Steve Blanchet , Z. Chacko , Rabindra N. Mohapatra

Heavy neutrinos with masses below the electroweak scale can simultaneously generate the light neutrino masses via the seesaw mechanism and the baryon asymmetry of the universe via leptogenesis. The requirement to explain these phenomena…

高能物理 - 唯象学 · 物理学 2017-09-13 Marco Drewes , Bjorn Garbrecht , Dario Gueter , Juraj Klaric

We discuss neutrino mass and mixing in the framework of the classic seesaw mechanism, involving right-handed neutrinos with large Majorana masses, which provides an appealing way to understand the smallness of neutrino masses. However, with…

高能物理 - 唯象学 · 物理学 2016-06-22 Stephen F. King

Neutrinos stand out among elementary particles through their unusually small masses. Various seesaw mechanisms attempt to explain this fact. In this work applying insights from matrix theory we are in a position to treat variants of seesaw…

高能物理 - 唯象学 · 物理学 2020-09-04 Wojciech Flieger , Janusz Gluza

A beautiful understanding of the smallness of the neutrino masses may be obtained via the seesaw mechanism, whereby one takes advantage of the key qualitative distinction between the neutrinos and the other fermions: right-handed neutrinos…

高能物理 - 唯象学 · 物理学 2015-06-03 Brian Feldstein , William Klemm

The type-I seesaw Lagrangian yields a non-generic set of active-sterile oscillation parameters - the neutrino mass eigenvalues and the physical elements of the full mixing matrix are entwined. For this reason one is able to, in principle,…

高能物理 - 唯象学 · 物理学 2013-05-30 Andre de Gouvea , Wei-Chih Huang

The seesaw mechanism of neutrino mass generation is analysed under the following assumptions: (1) minimal seesaw with no Higgs triplets, (2) hierarchical Dirac masses of neutrinos, (3) large lepton mixing primarily or solely due to the…

高能物理 - 唯象学 · 物理学 2008-11-26 E. Kh. Akhmedov

A novel scenario is presented within the Type-I seesaw mechanism in which no other beyond Standard Model fields except three heavy right handed neutrinos, have been considered. Light neutrino masses around sub eV scale, could be possible at…

高能物理 - 唯象学 · 物理学 2024-11-26 Kunal Pandey , Rathin Adhikari

We point out that the minimal seesaw model can provide a natural framework to accommodate tiny neutrino masses, while its experimental testability and notable predictiveness are still maintained. This possibility is based on the observation…

高能物理 - 唯象学 · 物理学 2010-05-12 He Zhang , Shun Zhou

The atmospheric and solar neutrino oscillation data suggest hierarchical neutrino masses with at least one large mixing. The simplest see-saw models for reconciling the two features are U(1) extensions of the SM with flavour dependent gauge…

高能物理 - 唯象学 · 物理学 2009-10-31 D. P. Roy
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