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相关论文: Baryogenesis at the electroweak phase transition

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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 investigate the evolution of the electroweak phase transition, using a one-Higgs effective potential that can be regarded as an approximation for the Minimal Supersymmetric Standard Model. The phase transition occurs in a small interval…

高能物理 - 唯象学 · 物理学 2009-10-31 Ariel Megevand

Electroweak Baryogenesis is a particularly attractive theoretical scenario, since it relies on physics which can be tested at present high energy collider facilities. Within the Standard Model, it has been shown that the requirement of…

高能物理 - 唯象学 · 物理学 2016-11-03 M. Carena , C. E. M. Wagner

Existence and properties of the electroweak phase transition in the early universe depend strongly on the mass of the Higgs scalar M_H. There is presumably no true symmetry restoration at high temperature. Nevertheless, a first order phase…

高能物理 - 唯象学 · 物理学 2008-02-03 Bastian Bergerhoff , Christof Wetterich

Standard theories of electroweak interactions are based on the concept of a gauge symmetry broken by the Higgs mechanism. If they are placed in an environment with a sufficiently high temperature, the symmetry gets restored. It turns out…

高能物理 - 唯象学 · 物理学 2017-08-23 M. Laine

The baryon density which may be produced during the electroweak phase transition in supersymmetric models is computed, taking into account the previously neglected effects of transport, strong and weak anomalous fermion number violation,…

高能物理 - 唯象学 · 物理学 2009-10-28 Patrick Huet , Ann E. Nelson

We compute the complete one-loop finite temperature effective potential for electroweak symmetry breaking in the Standard Model with a Higgs potential supplemented by higher dimensional operators as generated for instance in composite Higgs…

高能物理 - 唯象学 · 物理学 2008-11-26 C. Delaunay , C. Grojean , J. D. Wells

Cold electroweak baryogenesis was proposed as a scenario to bypass generic problems of electroweak baryogenesis within the Standard Model. In this scenario, baryogenesis takes place during an electroweak symmetry breaking transition, which…

高能物理 - 唯象学 · 物理学 2009-11-11 Anders Tranberg , Jan Smit

Electroweak baryogenesis (EWBG) remains a theoretically attractive and experimentally testable scenario for explaining the cosmic baryon asymmetry. We review recent progress in computations of the baryon asymmetry within this framework and…

高能物理 - 唯象学 · 物理学 2015-06-05 David E. Morrissey , Michael J. Ramsey-Musolf

We investigate scenarios in which electroweak baryogenesis can occur during an exotic stage of electroweak symmetry breaking in the early Universe. This transition is driven by the expectation value of a new electroweak scalar instead of…

高能物理 - 唯象学 · 物理学 2015-08-20 Nikita Blinov , Jonathan Kozaczuk , David E. Morrissey , Carlos Tamarit

Electroweak baryogenesis is an interesting theoretical scenario, which demands physics beyond the Standard Model at energy scales of the order of the weak boson masses. It has been recently emphasized that, in the presence of light stops,…

高能物理 - 唯象学 · 物理学 2016-09-06 M. Carena , M. Quiros , A. Riotto , I. Vilja , C. E. M. Wagner

We compute the baryon asymmetry generated at the electroweak phase transition by the Higgs scalar sector of the minimal supersymmetric standard model. Because of large enhancement effects from low momentum modes, Higgs particles may be…

高能物理 - 唯象学 · 物理学 2009-10-30 Antonio Riotto

We discuss the possibility of generating the baryon asymmetry of the Universe when the temperature of the Universe is much below the electroweak scale. In our model the evaporation of primordial black holes or the decay of massive particles…

高能物理 - 唯象学 · 物理学 2011-05-23 Raghavan Rangarajan , Supratim Sengupta , Ajit M. Srivastava , ;

The electroweak symmetry breaking transition may supply the appropriate out-of-equilibrium conditions for baryogenesis if it is triggered sufficiently fast. This can happen at the end of low-scale inflation, prompting baryogenesis to occur…

高能物理 - 唯象学 · 物理学 2010-10-27 Anders Tranberg , Jan Smit , Mark Hindmarsh

The mechanism of "cold electroweak baryogenesis" has been so far unpopular because its proposal has relied on the ad-hoc assumption of a period of hybrid inflation at the electroweak scale with the Higgs acting as the waterfall field. We…

高能物理 - 唯象学 · 物理学 2015-05-28 Thomas Konstandin , Geraldine Servant

We discuss the constraints on the Higgs sector coming from the requirement of the generation of the matter-antimatter asymmetry at the electroweak phase transition. These relate to both a strongly first order first transition, necessary for…

高能物理 - 唯象学 · 物理学 2023-11-14 Carlos E. M. Wagner

We consider the baryogenesis picture in the Zee-Babu model. Our analysis shows that electroweak phase transition (EWPT) in the model is a first-order phase transition at the $100$ GeV scale, its strength ranges from 1 to 4.15 and the masses…

高能物理 - 唯象学 · 物理学 2018-06-12 Vo Quoc Phong , Nguyen Chi Thao , Hoang Ngoc Long

We address electroweak baryogenesis in the context of composite Higgs models, pointing out that modifications to the Higgs and top quark sectors can play an important role in generating the baryon asymmetry. Our main observation is that…

高能物理 - 唯象学 · 物理学 2015-05-30 Jose R. Espinosa , Ben Gripaios , Thomas Konstandin , Francesco Riva

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 study the interactions of quarks and antiquarks with the changing Higgs field during the electroweak phase transition, including quantum mechanical and some thermal effects, with the only source of CP violation being the known CKM phase.…

高能物理 - 唯象学 · 物理学 2010-11-01 Glennys R. Farrar , M. E. Shaposhnikov
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