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相关论文: Nucleosynthesis Constraints on Defect-Mediated Ele…

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We perform an analysis of the behaviour of the electroweak phase transition in the Minimal Supersymmetric Standard Model, in the presence of light stops. We show that, in previously unexplored regions of parameter space, the order parameter…

高能物理 - 唯象学 · 物理学 2008-11-26 M. Carena , M. Quiros , C. E. M. Wagner

Electroweak baryogenesis could be very efficient at the end of an electroweak-scale inflation. Reheating that followed inflation could create a highly non-equilibrium plasma, in which the baryon number violating transitions were rapid. In…

高能物理 - 唯象学 · 物理学 2007-05-23 Alexander Kusenko

We construct a model for delayed electroweak symmetry breaking that takes place in a cold Universe with T<<100 GeV and which proceeds by a fast quench rather than by a conventional, slow, phase transition. This is achieved by coupling the…

宇宙学与河外天体物理 · 物理学 2014-11-21 Kari Enqvist , Philip Stephens , Olli Taanila , Anders Tranberg

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

We investigate the effects of baryon/anti-baryon inhomogeneity on primordial nucleosynthesis. Recent work claims that electroweak baryogenesis could give rise to distinct regions of net baryon and anti-baryon number, which could survive…

天体物理学 · 物理学 2007-05-23 Kevork Abazajian , George M. Fuller

We consider feasibility of electroweak baryogenesis in gauge mediated supersymmetry breaking models with messenger-matter mixing. We present a class of models where electroweak baryogenesis produces sufficient amount of baryon asymmetry.…

高能物理 - 唯象学 · 物理学 2011-07-19 D. S. Gorbunov

We propose a new alternative for baryogenesis which resolves a number of the problems associated with GUT and electroweak scenarios, and which may allow baryogenesis even in modest extensions of the standard model. If the universe never…

高能物理 - 唯象学 · 物理学 2009-10-31 Lawrence M. Krauss , Mark Trodden

We consider the effects of particle transport in the topological defect-mediated electroweak baryogenesis scenarios of Ref. 1. We analyze the cases of both thin and thick defects and demonstrate an enhancement of the original mechanism in…

高能物理 - 唯象学 · 物理学 2010-11-01 Robert Brandenberger , Anne-Christine Davis , Tomislav Prokopec , Mark Trodden

A possible solution to the observed baryon asymmetry in the universe is described, based on the physics of the standard model of electroweak interactions. At temperatures high enough electroweak physics provides violation of baryon number,…

高能物理 - 唯象学 · 物理学 2007-05-23 Nicholas Petropoulos

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

We demonstrate the viability of electroweak baryogenesis scenarios in which the necessary departure from equilibrium is realized by the evolution of a network of topological defects. We consider several effective models of TeV physics, each…

高能物理 - 唯象学 · 物理学 2010-11-01 M. Trodden , A-C. Davis , R. Brandenberger

Electroweak baryogenesis has become a topic of much recent activity [1]. Here we discuss a new scenario which has the advantage of being insensitive to the order of the electroweak phase transition. We briefly review a mechanism [2] using…

高能物理 - 唯象学 · 物理学 2009-09-25 A. C. Davis , R. Brandenberger , M. Trodden

Electroweak baryogenesis can occur in the ``adiabatic limit,'' in which expanding bubbles of true vacuum are assumed to have rather thick walls and be slowly moving. Here the problem of calculating the baryon asymmetry in this limit is…

高能物理 - 唯象学 · 物理学 2009-10-28 Michael Dine , Scott Thomas

It is known that baryon number inhomogeneities may arise as a consequence of electroweak baryogenesis. Their geometry, size, and amplitude depend on the parameters that characterize the baryogenesis mechanism, as well as on those that…

高能物理 - 唯象学 · 物理学 2009-11-10 Ariel Megevand , Francisco Astorga

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 , ;

We investigate baryogenesis from dark matter oscillations in the ultraviolet freeze-in regime. We find that the mechanism can simultaneously accommodate the observed abundances of baryons and dark matter for dark matter masses in the 10 keV…

高能物理 - 唯象学 · 物理学 2026-01-23 Tian Dong , Conor M. Floyd , Antonia Hekster , Derek J. Li , Brian Shuve , David Tucker-Smith

We analyze electroweak baryogenesis during a two-step electroweak symmetry breaking transition, wherein the baryon asymmetry is generated during the first step and preserved during the second. Focusing on the dynamics of CP-violation…

高能物理 - 唯象学 · 物理学 2016-01-27 Satoru Inoue , Grigory Ovanesyan , Michael J. Ramsey-Musolf

If stable electroweak strings are copiously produced during the electroweak phase transition, they may contribute significantly to the presently observed baryon to entropy ratio of the universe. This analysis establishes the feasibility of…

高能物理 - 唯象学 · 物理学 2007-05-23 Robert H. Brandenberger , Anne-Christine Davis

We consider the presence of cosmic string induced density fluctuations in the universe at temperatures below the electroweak phase transition temperature. Resulting temperature fluctuations can restore the electroweak symmetry locally,…

高能物理 - 唯象学 · 物理学 2009-11-07 Biswanath Layek , Soma Sanyal , Ajit M. Srivastava

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