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相关论文: The Origin of Neutrino Masses and Physics Beyond t…

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Theories in which neutrino masses are generated by a conventional see-saw mechanism generically yield masses which are O(v^2) in units where M_{Pl}=1, which is naively too small to explain the results from SuperKamiokande. In supersymmetric…

高能物理 - 唯象学 · 物理学 2007-05-23 Nima Arkani-Hamed , Lawrence Hall , Hitoshi Murayama , David Smith , Neal Weiner

If neutrino masses are obtained via the canonical seesaw mechanism, based on an underlying 2X2 mass matrix, unitarity violation of the neutrino mixing matrix is unavoidable, but its effect is extremely small. On the other hand, in the…

高能物理 - 唯象学 · 物理学 2010-11-15 Ernest Ma

We consider the problem of neutrino masses and mixing in the framework of flipped SU(5). The right-handed neutrino mass, generated through the operation of a seesaw mechanism by a sector of gauge singlets, leads naturally, at a subsequent…

高能物理 - 唯象学 · 物理学 2010-04-30 J. Rizos , K. Tamvakis

We study the origin of neutrino mass from $SO(10)$ arising from $M$ Theory compactified on a $G_2$-manifold. This is linked to the problem of the breaking of the extra $U(1)$ gauge group, in the $SU(5)\times U(1)$ subgroup of $SO(10)$,…

高能物理 - 唯象学 · 物理学 2016-12-21 Bobby S. Acharya , Krzysztof Bozek , Miguel Crispim Romão , Stephen F. King , Chakrit Pongkitivanichkul

Radiative neutrino mass generation within supersymmetric (SUSY) construction is studied. The mechanism is considered where the lepton number violation is originating from the soft SUSY breaking terms. This requires MSSM extensions with…

高能物理 - 唯象学 · 物理学 2017-01-04 Luka Megrelidze , Zurab Tavartkiladze

New effects related to refraction of neutrinos in different media are reviewed and implication of the effects to neutrino mass and mixing are discussed. Patterns of neutrino masses and mixing implied by existing hints/bounds are described.…

高能物理 - 唯象学 · 物理学 2008-02-03 Alexei Yu. Smirnov

In this work we show that we can generate neutrino masses through the type-II see-saw mechanism working at TeV scale in the context of a 331 model.

高能物理 - 唯象学 · 物理学 2014-11-17 J. C. Montero , C. A. de S. Pires , V. Pleitez

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

The neutrino oscillations are studied in the framework of the minimal supersymmetric SO(10) model with Type-III see-saw mechanism by additionally introducing a number of SO(10) singlet neutrinos. The light Majorana neutrino mass matrix is…

高能物理 - 唯象学 · 物理学 2009-11-11 Takeshi Fukuyama , Amon Ilakovac , Tatsuru Kikuchi , Koichi Matsuda

Knowledge of the mechanism of neutrino mass generation would help understand a lot more about Lepton Number Violation (LNV), the cosmological evolution of the Universe, or the evolu tion of astronomical objects. Here we propose a verifiable…

高能物理 - 唯象学 · 物理学 2020-03-18 Claudio Dib , Sergey Kovalenko , Ivan Schmidt , Adam Smetana

In this short talk, we present a renormalizable model that can i) generate neutrino masses via a low-scale seesaw mechanism and ii) solve the long-standing $(g-2)_\mu$ and the more recent CDF II $M_W$-anomalies. This is minimally achieved…

高能物理 - 唯象学 · 物理学 2023-04-18 A. de Giorgi , L. Merlo , S. Pokorski

The linear seesaw mechanism provides a simple way to generate neutrino masses. In addition to Standard Model particles, it includes quasi-Dirac leptons as neutrino mass mediators, and a leptophilic scalar doublet seeding small neutrino…

高能物理 - 唯象学 · 物理学 2023-08-21 Aditya Batra , Praveen Bharadwaj , Sanjoy Mandal , Rahul Srivastava , José W. F. Valle

Generation of neutrino mass in SO(4) model is proposed here. The algebraic structure of SO(4) is same as to that of $SU(2)_{L}\times SU(2)_{R}$. It is shown that the spontaneous symmetry breaking results three massive as well as three…

高能物理 - 唯象学 · 物理学 2014-11-18 Indranath Bhattacharyya

In this talk we show how a natural neutrino mass hierarchy can follow from the type I see-saw mechanism, and a natural neutrino mass degeneracy from the type II see-saw mechanism, where the bi-large mixing angles can arise from either the…

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

We consider a minimal formulation of SO(10) Grand Unified Theory wherein all the fermion masses arise from Yukawa couplings involving one 126 and one 10 of Higgs multiplets. It has recently been recognized that such theories can explain,…

高能物理 - 唯象学 · 物理学 2014-11-18 K. S. Babu , Cosmin Macesanu

Superstring derived $\E$ models can accommodate small neutrino masses if a discrete symmetry is imposed which forbids tree level Dirac neutrino masses but allows for radiative mass generation. The only possible symmetries of this kind are…

高能物理 - 唯象学 · 物理学 2009-09-25 Enrico Nardi

The minimal 3-3-1 model is perturbative until energies around 4-5TeV, posing a challenge to generate neutrino masses at eV scale, mainly if one aims to take advantage of the seesaw mechanism. As a means to circumvent this problem we propose…

高能物理 - 唯象学 · 物理学 2013-05-30 W. Caetano , D. Cogollo , C. A. de S. Pires , P. S. Rodrigues da Silva

In pursuit of a balance between theoretical naturalness and experimental testability, we propose two classes of multiple seesaw mechanisms at the TeV scale to understand the origin of tiny neutrino masses. They are novel extensions of the…

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

Neutrino masses arise via a seesaw mechanism and its mass hierarchy, with assumption that heavy Majorana neutrino mass matrix subject to $\mu-\tau$ symmetry and invariant under a cyclic permutation, are evaluated. Within this scenario, the…

高能物理 - 唯象学 · 物理学 2010-06-03 Asan Damanik

The theory that the extra-space component of the gauge field is identified with the standard model Higgs boson, is called the gauge-Higgs unification (GHU) scenario. We examine how the small neutrino masses are naturally generated in the…

高能物理 - 唯象学 · 物理学 2019-04-30 K. Hasegawa