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相关论文: Leptogenesis, Dark Energy, Dark Matter and the neu…

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We propose a model with an $U(1)_{B-L}$ gauge symmetry, in which small neutrino masses, dark matter and the matter-antimatter asymmetry in the Universe can be simultaneously explained. In particular, the neutrino masses are generated…

高能物理 - 唯象学 · 物理学 2018-02-19 Chao-Qiang Geng , Hiroshi Okada

It is proposed that dark matter is the origin of neutrino mass, thereby linking inexorably two undisputed (and seemingly unrelated) pieces of evidence for physics beyond the Standard Model. Leptogenesis at the TeV scale may also be…

高能物理 - 唯象学 · 物理学 2008-11-26 Ernest Ma

The discovery of neutrino oscillations provides a solid evidence for nonzero neutrino masses and leptonic mixing. The fact that neutrino masses are so tiny constitutes a puzzling problem in particle physics. From the theoretical viewpoint,…

高能物理 - 唯象学 · 物理学 2015-05-30 R. Gonzalez Felipe

Properties of neutrinos may be the origin of the matter-antimatter asymmetry of the universe. In the seesaw model for neutrino masses this leads to important constraints on the properties of light and heavy neutrinos. In particular, an…

高能物理 - 唯象学 · 物理学 2011-08-17 W. Buchmuller , P. Di Bari , M. Plumacher

Radiative neutrino mass models have interesting features, which make it possible to relate neutrino masses to the existence of dark matter. However, the explanation of the baryon number asymmetry in the universe seems to be generally…

高能物理 - 唯象学 · 物理学 2015-03-17 H. Higashi , T. Ishima , D. Suematsu

We propose a unified explanation for the origin of dark matter and baryon number asymmetry on the basis of a non-supersymmetric model for neutrino masses. Neutrino masses are generated in two distinct ways, that is, a tree-level seesaw…

高能物理 - 唯象学 · 物理学 2008-11-26 Daijiro Suematsu

By extending the lepton sector of standard model to include one sterile neutrino and two sets of new Higgs doublets and right-handed neutrinos, denoted by $(\eta_1, N_1, N_3)$ and $(\eta_2, N_2, N_4)$, with two $Z_2$ symmetries, the puzzles…

高能物理 - 唯象学 · 物理学 2009-05-26 Chuan-Hung Chen

We propose a new model to explain the neutrino masses, the dark energy and the baryon asymmetry altogether. In this model, neutrinos naturally acquire small Majorana masses via type-II seesaw mechanism, while the pseudo-Nambu-Goldstone…

高能物理 - 唯象学 · 物理学 2008-11-26 Pei-Hong Gu , Hong-Jian He , Utpal Sarkar

We propose a minimal model based on lepton number symmetry (and violation), to address a common origin of baryon asymmetry, dark matter and neutrino mass generation. The model consists of a vector like fermion to constitute the dark sector,…

高能物理 - 唯象学 · 物理学 2022-10-12 Subhaditya Bhattacharya , Rishav Roshan , Arunansu Sil , Drona Vatsyayan

We present a new realization of asymmetric dark matter in which the dark matter and lepton asymmetries are generated simultaneously through two-sector leptogenesis. The right-handed neutrinos couple both to the Standard Model and to a…

高能物理 - 唯象学 · 物理学 2011-05-26 Adam Falkowski , Joshua T. Ruderman , Tomer Volansky

Neutrino properties can play a crucial role in determining the matter-antimatter asymmetry of the universe if thermal leptogenesis is the correct solution to the baryogenesis problem. Owing to this, the study of neutrino models goes beyond…

高能物理 - 唯象学 · 物理学 2009-01-12 Sandy S. C. Law

The Standard Model (SM) is inadequate to explain the origin of tiny neutrino masses, the dark matter (DM) relic abundance and also the baryon asymmetry of the Universe. In this work to address all the three puzzles, we extend the SM by a…

高能物理 - 唯象学 · 物理学 2017-12-19 Anirban Biswas , Sandhya Choubey , Sarif Khan

We study a simple extension of the standard model to simultaneously explain neutrino masses, dark matter and the matter-antimatter asymmetry of the Universe. In our model, the baryon asymmetry is achieved by the leptogenesis mechanism,…

高能物理 - 唯象学 · 物理学 2010-03-26 Chuan-Hung Chen , Chao-Qiang Geng , Dmitry V. Zhuridov

We consider the possibility of simultaneously addressing the baryon asymmetry of the Universe, the dark matter problem and the neutrino mass generation in minimal extensions of the Standard Model via sterile fermions with (small) total…

高能物理 - 唯象学 · 物理学 2018-03-20 Asmaa Abada , Giorgio Arcadi , Valerie Domcke , Michele Lucente

We explore in some detail the hypothesis that the generation of a primordial lepton-antilepton asymmetry (Leptogenesis) early on in the history of the Universe is the root cause for the origin of matter. After explaining the theoretical…

高能物理 - 唯象学 · 物理学 2009-11-11 W. Buchmuller , R. D. Peccei , T. Yanagida

We investigate the possibility that dark matter and the baryon asymmetry of the Universe are generated by the same mechanism, following an idea initially proposed by V.A. Kuzmin and recently discussed by R. Kitano and I. Low. In our model,…

高能物理 - 唯象学 · 物理学 2009-11-11 Nicolas Cosme , Laura Lopez Honorez , Michel H. G. Tytgat

We propose a model of asymmetric dark matter (DM) where the dark sector is an identical copy of both forces and matter of the standard model (SM) as in the mirror universe models discussed in literature. In addition to being connected by…

高能物理 - 唯象学 · 物理学 2010-04-08 Haipeng An , Shao-Long Chen , Rabindra N. Mohapatra , Yue Zhang

Properties of neutrinos, the lightest of all elementary particles, may be the origin of the entire matter-antimatter asymmetry of the universe. This requires that neutrinos are Majorana particles, which are equal to their antiparticles, and…

高能物理 - 唯象学 · 物理学 2009-11-07 W. Buchmüller , P. Di Bari , M. Plümacher

Despite the lack of evidence of new physics at colliders, neutrino masses, dark matter and matter-antimatter asymmetry of the universe require an extension of the Standard Model. After discussing some new concepts and tools in the…

高能物理 - 唯象学 · 物理学 2019-05-10 Pasquale Di Bari

We propose a low scale leptogenesis scenario in the framework of composite Higgs models supplemented with singlet heavy neutrinos. One of the neutrinos can also be considered as a dark matter candidate whose stability is guaranteed by a…

高能物理 - 唯象学 · 物理学 2021-04-28 M. Ahmadvand
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