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相关论文: Sleptogenesis

200 篇论文

The possibility of generating the baryon asymmetry of the Universe via flavor oscillation in the early Universe is discussed. After the inflation, leptons are born in some states, travel in the medium, and are eventually projected onto…

高能物理 - 唯象学 · 物理学 2018-11-01 Yuta Hamada , Ryuichiro Kitano , Wen Yin

Mixing lepton doublets of the Standard Model can lead to lepton flavour asymmetries in the Early Universe. We present a diagrammatic representation of this recently identified source of $CP$ violation and elaborate in detail on the…

高能物理 - 唯象学 · 物理学 2015-12-09 Bjorn Garbrecht , Ignacio Izaguirre

Soft leptogenesis is a scenario in which the cosmic baryon asymmetry is produced from a lepton asymmetry generated in the decays of heavy sneutrinos (the partners of the singlet neutrinos of the seesaw) and where the relevant sources of CP…

高能物理 - 唯象学 · 物理学 2011-09-07 Chee Sheng Fong , M. C. Gonzalez-Garcia , Enrico Nardi

The baryon asymmetry of the universe can be explained by the out-of-equilibrium decays of heavy right-handed neutrinos. We analyse this mechanism in the framework of a supersymmetric extension of the Standard Model and show that lepton…

高能物理 - 唯象学 · 物理学 2007-05-23 M. Plumacher

If the expectation value of the right-handed (rhd) sneutrino comes to dominate the universe, its decay naturally leads to successful leptogenesis, as well as significant dilution of dangerous inflationary relics, such as the gravitino. The…

高能物理 - 唯象学 · 物理学 2009-02-20 A. Hebecker , J. March-Russell , T. Yanagida

We analyze lepton asymmetry induced in the decay of right--handed neutrinos in a class of minimal left--right symmetric models. In these models, which assume low energy supersymmetry, the Dirac neutrino mass matrix is proportional to the…

高能物理 - 唯象学 · 物理学 2015-06-25 K. S. Babu , A. Bachri , H. Aissaoui

We investigate the possibility that the entropy producing decay of a right-handed sneutrino condensate can simultaneously be the source of the baryon asymmetry, of gravitino dark matter, and of cosmological density perturbations. For…

高能物理 - 唯象学 · 物理学 2009-11-10 Rouzbeh Allahverdi , Manuel Drees

We consider a question which curiously had not been properly considered so far: in the standard seesaw model what is the minimum value the mass of a right-handed (RH) neutrino must have for allowing successful leptogenesis via CP-violating…

高能物理 - 唯象学 · 物理学 2016-08-29 Thomas Hambye , Daniele Teresi

The baryon asymmetry of the universe can be explained by the out-of-equilibrium decays of heavy right-handed neutrinos. We analyse this mechanism in the framework of a supersymmetric extension of the Standard Model and show that lepton…

高能物理 - 唯象学 · 物理学 2016-09-06 M. Plumacher

We consider the generation of the baryon asymmetry in models with right-handed neutrinos produced through gravitational scattering of the inflaton during reheating. The right-handed neutrinos later decay and generate a lepton asymmetry,…

高能物理 - 唯象学 · 物理学 2022-05-05 Raymond T. Co , Yann Mambrini , Keith A. Olive

We discuss aidnogenesis, the generation of a dark matter asymmetry via new sphaleron processes associated to an extra non-abelian gauge symmetry common to both the visible and the dark sectors. Such a theory can naturally produce an…

高能物理 - 唯象学 · 物理学 2011-03-07 Mattias Blennow , Basudeb Dasgupta , Enrique Fernandez-Martinez , Nuria Rius

We evaluate the constraints that the COBE observations put on baryogenesis in inflationary cosmologies.We consider the supersymmetric version of the proposal of Fukugita and Yanagida, that the baryon asymmetry of the universe is created by…

高能物理 - 唯象学 · 物理学 2009-09-15 B. A. Campbell , S. Davidson , K. A. Olive

In this work we study a classically scale invariant extension of the Standard Model that can explain simultaneously dark matter and the baryon asymmetry in the universe. In our set-up we introduce a dark sector, namely a non-Abelian SU(2)…

高能物理 - 唯象学 · 物理学 2016-11-23 Valentin V. Khoze , Alexis D. Plascencia

We calculate the baryonic asymmetry of the universe in the baryogenesis-via-leptogenesis framework, assuming first a quark-lepton symmetry and then a charged-neutral lepton symmetry. We match the results with the experimentally favoured…

高能物理 - 唯象学 · 物理学 2009-10-31 D. Falcone , F. Tramontano

We investigate in detail the leptogenesis by the decay of coherent right-handed sneutrino $\widetilde{N}$ having dominated the energy density of the early universe, which was originally proposed by HM and TY. Once the $\widetilde{N}$…

高能物理 - 唯象学 · 物理学 2009-09-29 K. Hamaguchi , Hitoshi Murayama , T. Yanagida

In order to address the baryon asymmetry in the Universe one needs to understand the origin of baryon (B) and lepton (L) number violation. In this article, we discuss the mechanism of baryogenesis via leptogenesis to explain the…

高能物理 - 唯象学 · 物理学 2021-09-10 Pavel Fileviez Perez , Clara Murgui , Alexis D. Plascencia

We study a class of leptogenesis scenarios with decay or scattering being the source of lepton asymmetry, which can not only give rise to the observed baryon asymmetry in the universe but also can leave behind a large remnant neutrino…

高能物理 - 唯象学 · 物理学 2023-08-14 Debasish Borah , Arnab Dasgupta

We discuss leptogenesis in a realistic supersymmetric model of inflation with a low reheat temperature 1-10 GeV. The lepton asymmetry is generated by a decaying right handed sneutrino, which is produced after inflation during preheating.…

高能物理 - 唯象学 · 物理学 2009-10-31 M. Bastero-Gil , S. F. King

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 review the experimental evidence for a net baryon density in cosmology, and the theoretical mechanism for producing it, called leptogenesis, which relies on the creation of a lepton asymmetry at an intermediate step. The naturality of…

高能物理 - 唯象学 · 物理学 2007-05-23 J. Orloff