Search results for "extensions of the standard model"

showing 5 items of 5 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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Observational constraints on decoupled hidden sectors

2016

We consider an extension of the Standard Model with a singlet sector consisting of a real (pseudo)scalar and a Dirac fermion coupled with the Standard Model only via the scalar portal. We assume that the portal coupling is weak enough for the singlet sector not to thermalize with the Standard Model allowing the production of singlet particles via the freeze-in mechanism. If the singlet sector interacts with itself sufficiently strongly, it may thermalize within itself, resulting in dark matter abundance determined by the freeze-out mechanism operating within the singlet sector. We investigate this scenario in detail. In particular, we show that requiring the absence of inflationary isocurva…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterScalar (mathematics)FOS: Physical sciencesParameter space114 Physical sciences01 natural sciencesStandard Modeldecouplingsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)ABELL 38270103 physical sciencesSinglet state010306 general physicsdark matter abundanceInflation (cosmology)PhysicsINTERACTING DARK-MATTERta114010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyextensions of the Standard ModelHidden sectorHigh Energy Physics - Phenomenologysinglet sectorCOSMOLOGICAL SIMULATIONSDirac fermionGALAXY CLUSTER 1E-0657-56symbols3.5 KEV LINEINTERACTION CROSS-SECTIONAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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Reheating the Standard Model from a hidden sector

2016

We consider a scenario where the inflaton decays to a hidden sector thermally decoupled from the visible Standard Model sector. A tiny portal coupling between the hidden and the visible sectors later heats the visible sector so that the Standard Model degrees of freedom come to dominate the energy density of the Universe before Big Bang Nucleosynthesis. We find that this scenario is viable, although obtaining the correct dark matter abundance and retaining successful Big Bang Nucleosynthesis is not obvious. We also show that the isocurvature perturbations constituted by a primordial Higgs condensate are not problematic for the viability of the scenario.

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Ultimate fate of the universereheatingmedia_common.quotation_subjectDark matterUNIVERSEFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics114 Physical sciences01 natural sciencesdark matterdecouplingpimeä aineHigh Energy Physics - Phenomenology (hep-ph)INFLATIONBig Bang nucleosynthesis0103 physical sciencesDARK-MATTERELECTROWEAK VACUUM010306 general physicsmedia_commonPhysicsQuintom scenariota114STABILITY010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyDecoupling (cosmology)InflatonHIGGSUniverseHidden sectorextensions of the Standard ModelHigh Energy Physics - Phenomenologyhidden sectorsSCALARAstrophysics - Cosmology and Nongalactic Astrophysics
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Baryogenesis in the two doublet and inert singlet extension of the Standard Model

2016

We investigate an extension of the Standard Model containing two Higgs doublets and a singlet scalar field (2HDSM). We show that the model can have a strongly first-order phase transition and give rise to the observed baryon asymmetry of the Universe, consistent with all experimental constraints. In particular, the constraints from the electron and neutron electric dipole moments are less constraining here than in pure two-Higgs-doublet model (2HDM). The two-step, first-order transition in 2HDSM, induced by the singlet field, may lead to strong supercooling and low nucleation temperatures in comparison with the critical temperature, $T_n \ll T_c$, which can significantly alter the usual pha…

Phase transitionCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciences7. Clean energy01 natural sciencesMolecular physicsStandard ModelHigh Energy Physics - Phenomenology (hep-ph)Baryon asymmetry0103 physical sciencescosmological phase transitionstwo-Higgs-doublet modelsSinglet state010306 general physicsPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and Astrophysicsextensions of the Standard ModelBaryogenesisHigh Energy Physics - Phenomenologyscalar fieldsHiggs bosonbaryon asymmetryScalar fieldAstrophysics - 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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