Search results for "electroweak phase transition"

showing 3 items of 3 documents

First Order Electroweak Phase Transition from (Non)Conformal Extensions of the Standard Model

2015

We analyse and compare the finite-temperature electroweak phase transition properties of classically (non)conformal extensions of the Standard Model. In the classically conformal scenarios the breaking of the electroweak symmetry is generated radiatively. The models feature new scalars coupled conformally to the Higgs sector as well as new fermions. We uncover the parameter space leading to a first order phase transition with(out) the Veltman conditions. We also discuss dark (matter) aspects of some of the models and compare with existing literature when appropriate. We observe that to accommodate both, a first order electroweak phase transition, and a phenomenologically viable dark matter …

High Energy Physics - TheoryNuclear and High Energy PhysicsPhase transitionParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard ModelDark matterFOS: Physical scienceshep-latTechnicolor7. Clean energy01 natural sciencesdark matterHiggs sectorStandard ModelHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Lattice0103 physical sciences010306 general physicsPhysicsta114010308 nuclear & particles physicshep-thHigh Energy Physics - Lattice (hep-lat)Electroweak interactionHigh Energy Physics::Phenomenologyhep-phSymmetry (physics)High Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)astro-ph.COelectroweak phase transitionextensions of the standard modelAstrophysics - Cosmology and Nongalactic Astrophysics
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A strong electroweak phase transition from the inflaton field

2016

We study a singlet scalar extension of the Standard Model. The singlet scalar is coupled non-minimally to gravity and assumed to drive inflation, and also couple sufficiently strongly with the SM Higgs field in order to provide for a strong first order electroweak phase transition. Requiring the model to describe inflation successfully, be compatible with the LHC data, and yield a strong first order electroweak phase transition, we identify the regions of the parameter space where the model is viable. We also include a singlet fermion with scalar coupling to the singlet scalar to probe the sensitivity of the constraints on additional degrees of freedom and their couplings in the singlet sec…

cosmological inflationParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard ModelScalar (mathematics)Degrees of freedom (physics and chemistry)FOS: Physical sciences01 natural sciences7. Clean energyStandard ModelGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsPhysicsInflation (cosmology)010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsInflatonextensions of the Standard ModelHiggs fieldHigh Energy Physics - Phenomenologyelectroweak phase transitionAstrophysics - Cosmology and Nongalactic Astrophysics
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Theories relating baryon asymmetry and dark matter

2014

The nature of dark matter and the origin of the baryon asymmetry are two of the deepest mysteries of modern particle physics. In the absence of hints regarding a possible solution to these mysteries, many approaches have been developed to tackle them simultaneously leading to very diverse and rich models. We give a short review where we describe the general features of some of these models and an overview on the general problem. We also propose a diagrammatic notation to label the different models.

PhysicsParticle physicsleptogenesisdark matterWIMP010308 nuclear & particles physicsMaterials Science (miscellaneous)General problemPhysicsDark matterBiophysicsGeneral Physics and AstronomyNotation01 natural sciencesDiagrammatic reasoningBaryon asymmetryLeptogenesisasymmetric dark matter0103 physical sciencesbaryon asymmetryddc:530electroweak phase transitionPhysical and Theoretical Chemistry010306 general physicsMathematical Physics
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