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Baryon asymmetry of the universe is generated in the supersymmetric standard model (SSM) through the charge transport mechanism mediated by top squarks. Necessary CP violation originates from a complex phase contained in mass-squared…

High Energy Physics - Phenomenology · Physics 2007-05-23 Mayumi Aoki , Noriyuki Oshimo

The Minimal Supersymmetric Standard Model has a candidate dark matter particle in its spectrum and may be able to generate the baryon asymmetry of the Universe (BAU) at the electroweak phase transition. In the Constrained MSSM, we find the…

High Energy Physics - Phenomenology · Physics 2009-10-31 Sacha Davidson , Toby Falk , Marta Losada

The standard requirement for the production of baryons at the electroweak phase transition, that the phase transition be first order and the sphaleron bound be satisfied, is predicated on the assumption of a radiation dominated universe at…

High Energy Physics - Phenomenology · Physics 2016-09-06 Michael Joyce

We consider the scenario of electroweak baryogenesis mediated by cosmological defect in models of supersymmetry breaking. When the effective electroweak breaking scale is raised in the defect configuration, the mechanism of electroweak…

High Energy Physics - Phenomenology · Physics 2014-11-17 Tomohiro Matsuda

A cosmological pseudoscalar field coupled to hypercharge topological number density can exponentially amplify hyperelectric and hypermagnetic fields while coherently rolling or oscillating, leading to the formation of a time-dependent…

High Energy Physics - Phenomenology · Physics 2009-10-31 Ram Brustein , David H. Oaknin

We show that certain models for neutrino masses that lead to the MSW explanation of the solar neutrino data and/or the hot dark matter component in the universe can also naturally allow for the successful generation of the cosmological…

High Energy Physics - Phenomenology · Physics 2009-09-17 J. T. Peltoniemi , J. W. F. Valle

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…

High Energy Physics - Phenomenology · Physics 2009-10-28 Michael Dine , Scott Thomas

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…

High Energy Physics - Phenomenology · Physics 2009-09-25 A. C. Davis , R. Brandenberger , M. Trodden

We present the computation of the baryon asymmetry in the SM amplified by dimension-6 Higgs interactions using the WKB approximation. Analyzing the one-loop potential it turns out that the phase transition is strongly first order in a wide…

High Energy Physics - Phenomenology · Physics 2015-06-25 Lars Fromme

A review of the present state of the baryogenesis is given with an emphasis on electroweak baryogenesis. Technical details of the numerous models cosidered in the literature are not elaborated but unresolved problems of the issue are…

High Energy Physics - Phenomenology · Physics 2010-11-01 A. D. Dolgov

We present arguments that the CKM CP-violation in the standard model may be sufficient for the generation of the baryon asymmetry, if the electroweak transition in the early universe was of the cold, tachyonic, type after electroweak-scale…

High Energy Physics - Phenomenology · Physics 2017-08-23 Jan Smit

We provide an up to date account of progress in understanding the origin of the observed baryon asymmetry of the universe. While our primary goal is to be current, we have attempted to give a pedagogical introduction to the primary areas of…

High Energy Physics - Phenomenology · Physics 2009-07-09 Antonio Riotto , Mark Trodden

The Standard Model of Particle Physics cannot explain the observed baryon asymmetry of the Universe. This observation is a clear sign of new physics beyond the Standard Model. There have been many recent theoretical developments to address…

We demonstrate that $CP-$violation in the Majorana mass matrices of the heavy neutrinos can generate a $CP-$asymmetric universe. The subsequent decay of the Majorana particles generates a lepton number asymmetry. During the electroweak…

High Energy Physics - Phenomenology · Physics 2010-11-01 Marion Flanz , Emmanuel A. Paschos , Utpal Sarkar

Majorana masses of the neutrino implies lepton number violation and is intimately related to the lepton asymmetry of the universe, which gets related to the baryon asymmetry of the universe in the presence of the sphalerons during the…

High Energy Physics - Phenomenology · Physics 2009-10-31 Utpal Sarkar

We study the possibility of baryogenesis in the case of supersymmetry breaking with large mixing between the right-handed scalar charm and right-handed scalar top or right-handed scalar up and right-handed scalar top squarks resulting in…

High Energy Physics - Phenomenology · Physics 2016-08-24 Mihir P. Worah

Electroweak baryogenesis is addressed within the context of the standard model of particle physics. Although the minimal standard model has the means of fulfilling the three Sakharov's conditions, it falls short to explaining the making of…

High Energy Physics - Phenomenology · Physics 2008-02-03 Patrick Huet

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…

High Energy Physics - Phenomenology · Physics 2009-11-10 Ariel Megevand , Francisco Astorga

We study the generation of the baryon asymmetry in a variant of the standard model, where the Higgs field is stabilized by a dimension-six interaction. Analyzing the one-loop potential, we find a strong first order electroweak phase…

High Energy Physics - Phenomenology · Physics 2008-11-26 Dietrich Bodeker , Lars Fromme , Stephan J. Huber , Michael Seniuch

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…

High Energy Physics - Phenomenology · Physics 2010-10-27 Anders Tranberg , Jan Smit , Mark Hindmarsh
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