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相关论文: Baryon Asymmetry and Neutrino Mixing

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Baryogenesis appears to require lepton number violation. This is naturally realized in extensions of the standard model containing right-handed neutrinos. We discuss the generation of a baryon asymmetry by the out-of-equilibrium decay of…

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

Baryogenesis appears to require lepton number violation. This is naturally realized in extensions of the standard model containing right-handed neutrinos. We discuss the generation of a baryon asymmetry by the out-of-equilibrium decay of…

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

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

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

Due to sphaleron processes in the high-temperature symmetric phase of the standard model the cosmological baryon asymmetry is related to neutrino properties. For hierarchical neutrino masses, with $B-L$ broken at the unification scale…

高能物理 - 唯象学 · 物理学 2008-11-26 W. Buchmüller , M. Plümacher

The cosmological baryon asymmetry can be explained as remnant of heavy Majorana neutrino decays in the early universe. We study this mechanism for two models of neutrino masses with a large \nu_\mu-\nu_\tau mixing angle which are based on…

高能物理 - 唯象学 · 物理学 2009-10-31 W. Buchmuller , M. Plumacher

The cosmological baryon asymmetry can be explained by the nonperturbative electroweak reprocessing of a lepton asymmetry generated in the out-of-equilibrium decay of heavy right-handed Majorana neutrinos. We analyze this mechanism in detail…

高能物理 - 唯象学 · 物理学 2007-05-23 Michael Pluemacher

In the standard model and most of its extensions the electroweak transition is too weak to affect the cosmological baryon asymmetry. Due to sphaleron processes baryogenesis in the high-temperature, symmetric phase of the standard model is…

高能物理 - 唯象学 · 物理学 2007-05-23 W. Buchmüller

A large neutrino asymmetry is an interesting possibility for cosmology, which can have significant observable consequences for nucleosynthesis and the cosmic microwave background. However, although it is a possibility, there is no obvious…

高能物理 - 唯象学 · 物理学 2009-10-31 John McDonald

The presently observed cosmological baryon asymmetry has been finally determined at the time of the electroweak phase transition, when baryon and lepton number violating interactions fell out of thermal equilibrium. We discuss the…

高能物理 - 唯象学 · 物理学 2007-05-23 W. Buchmuller

We reconsider the GUT-baryogenesis mechanism for generating the baryon asymmetry of the Universe. The baryon asymmetry is produced by the out of equilibrium decay of coloured Higgs bosons at the GUT scale, conserving B-L. If neutrinos are…

高能物理 - 唯象学 · 物理学 2007-05-23 J. A. Lopez-Perez , N. Rius

Cosmological baryon asymmetry B is studied in supersymmetric standard models, assuming the electroweak reprocessing of B and L. Only when the soft supersymmetry breaking is taken into account, B is proportional to the primordial B-L in the…

高能物理 - 唯象学 · 物理学 2009-10-22 T. Inui , T. Ichihara , Y. Mimura , N. Sakai

The difference between baryon number B and lepton number L is the only anomaly-free global symmetry of the Standard Model, easily promoted to a local symmetry by introducing three right-handed neutrinos, which automatically make neutrinos…

高能物理 - 唯象学 · 物理学 2014-11-11 Julian Heeck

The lepton asymmetry created in the out-of-equilibrium decay of a heavy Majorana neutrino can generate the cosmological baryon asymmetry when processed through fast anomalous electroweak reactions. In this work I examine this process under…

高能物理 - 唯象学 · 物理学 2014-11-17 Haim Goldberg

The mass hierarchies of quarks and charged leptons as well as a large $\n_\m$-$\n_\t$ mixing angle are naturally explained by the Frogatt-Nielsen mechanism with a nonparallel family structure of chiral charges. We extend this mechanism to…

高能物理 - 唯象学 · 物理学 2009-10-31 W. Buchmüller , T. Yanagida

We propose a resonant leptogenesis scenario in a U(1)_{B-L} gauge extension of the standard model to generate large lepton asymmetries for cosmological baryon asymmetry and dark matter. After B-L number is spontaneously broken, inflaton can…

高能物理 - 唯象学 · 物理学 2010-12-09 Pei-Hong Gu

A mechanism is presented, in which the mixing of right handed heavy Majorana neutrinos creates a $CP-$asymmetric universe. When these Majorana neutrinos subsequently decay more leptons than anti-leptons are produced. The lepton asymmetry…

高能物理 - 唯象学 · 物理学 2009-10-28 Marion Flanz , Emmanuel A. Paschos , Utpal Sarkar , Jan Weiss

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 put forward a new proposal for generating the baryon asymmetry of the universe by making use of the dynamics of a $\mathrm{U}(1)$ scalar field coupled to dark matter. High dark matter densities cause the $\mathrm{U}(1)$ symmetry to break…

高能物理 - 唯象学 · 物理学 2017-11-22 Jeremy Sakstein , Mark Trodden

We discuss the various incarnations of a gauged B-L symmetry: 1) unbroken, it features Dirac neutrinos, neutrinogenesis to create the baryon asymmetry of our Universe, and a potentially light Z' boson; 2) broken by two units, we obtain the…

高能物理 - 唯象学 · 物理学 2015-03-27 Julian Heeck
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