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相关论文: Supersymmetry Protects the Primordial Baryon Asymm…

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We discuss two independent issues about the baryon asymmetry of the universe. First, assuming that it is generated by an unspecified source at high temperatures, we study the effects of non-perturbative $SU(2)_W$ dynamics above the…

高能物理 - 唯象学 · 物理学 2009-10-22 Luis E. Ibanez , Fernando Quevedo

We note that the maximum temperature during reheating can be much greater than the reheating temperature $T_r$ at which the Universe becomes radiation dominated. We show that the Standard Model anomalous $(B+L)$-violating processes can…

高能物理 - 唯象学 · 物理学 2009-10-31 Sacha Davidson , Marta Losada , Antonio Riotto

In the presence of anomaly induced sphaleron process, only a B-L asymmetry can be partially converted to the baryon asymmetry while any B+L asymmetry would be completely erased. Thus in any successful baryogenesis theories, B-L is usually…

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

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

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

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 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

Requiring that the baryon number of the universe be generated by anomalous electroweak interactions places strong constraints on the minimal supersymmetric standard model. In particular, the electric dipole moment of the neutron must be…

高能物理 - 唯象学 · 物理学 2010-11-01 A. Cohen , A. Nelson

We show that "accidental" supersymmetry is a beyond-the-Standard Model framework that naturally accommodates a thermal relic dark matter candidate and successful electroweak baryogenesis, including the needed strongly first-order character…

高能物理 - 唯象学 · 物理学 2015-06-11 Jonathan Kozaczuk , Stefano Profumo , Carroll L. Wainwright

The Standard Model (SM) of particle physics is a precise model of electroweak interactions, however there is growing tension between the SM and observations (neutrino oscillations, dark matter, dark energy, baryogenesis, among others).…

高能物理 - 唯象学 · 物理学 2016-08-23 Zachary Burell

The origin of the matter-antimatter asymmetry of the universe remains one of the outstanding questions yet to be answered by modern cosmology and also one of only a handful of problems where the need of a larger number of degrees of freedom…

高能物理 - 唯象学 · 物理学 2017-08-23 Gabriella Piccinelli , Alejandro Ayala

Primordial Big-Bang Nucleosynthesis (BBN) tightly constrains the existence of any additional relativistic degrees of freedom at that epoch. However a large asymmetry in electron neutrino number shifts the chemical equilibrium between the…

高能物理 - 唯象学 · 物理学 2009-10-31 J. March-Russell , H. Murayama , A. Riotto

In principle, the baryon asymmetry of the Universe can be generated at the electroweak phase transition but the experimental lower limit on the Higgs mass seems to rule out a Standard Model scenario. However, it has been shown recently that…

高能物理 - 唯象学 · 物理学 2009-02-16 D. Delepine

We consider the impact of cosmological $B-L$ constraints on supersymmetric standard models with bilinear breaking of R-parity. In order to avoid erasing any primordial baryon or lepton asymmetry above the electroweak scale, $B-L$ violation…

高能物理 - 唯象学 · 物理学 2014-11-17 A. G. Akeroyd , E. J. Chun , M. A. Diaz , D. -W. Jung

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 realisation that the electroweak anomaly can induce significant baryon number violation at high temperature and that the standard models of particle physics and cosmology contain all the ingredients needed for baryogenesis has led to…

高能物理 - 唯象学 · 物理学 2009-09-25 U. A. yajnik

We consider a minimal supersymmetric extension of the Standard Model, with right-handed neutrinos and local B-L, the difference between baryon and lepton number, a symmetry which is spontaneously broken at the scale of grand unification. To…

高能物理 - 唯象学 · 物理学 2015-04-09 Wilfried Buchmüller , Valerie Domcke , Kohei Kamada , Kai Schmitz

The simplest interpretation of the global success of the Standard Model is that new physics decouples well above the electroweak scale. Supersymmetric extension of the Standard Model offers the possibility of light chargino and the…

高能物理 - 唯象学 · 物理学 2009-10-28 P. H. Chankowski , S. Pokorski

As a result of the Standard Model chiral anomalies, baryon number is violated in the early universe in the presence of a hypermagnetic field with varying helicity. We investigate whether the matter / anti-matter asymmetry of the universe…

宇宙学与河外天体物理 · 物理学 2016-09-14 Kohei Kamada , Andrew J. Long

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
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