0000000000417617

AUTHOR

Stanislav Rusak

0000-0002-0168-8447

showing 4 related works from this author

Postinationary vacuum instability and Higgs-inflaton couplings

2016

The Higgs-inflaton coupling plays an important role in the Higgs field dynamics in the early Universe. Even a tiny coupling generated at loop level can have a dramatic effect on the fate of the electroweak vacuum. Such Higgs-inflaton interaction is present both at the trilinear and quartic levels in realistic reheating models. In this work, we examine the Higgs dynamics during the preheating epoch, focusing on the effects of the parametric and tachyonic resonances. We use lattice simulations and other numerical tools in our studies. We find that the resonances can induce large fluctuations of the Higgs field which destabilize the electroweak vacuum. Our considerations thus provide an upper …

General Relativity and Quantum CosmologyHiggs-inflation couplingsHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyHigh Energy Physics::ExperimentAstrophysics::Cosmology and Extragalactic Astrophysics
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Lattice Calculation of the Decay of Primordial Higgs Condensate

2015

We study the resonant decay of the primordial Standard Model Higgs condensate after inflation into $SU(2)$ gauge bosons on the lattice. We find that the non-Abelian interactions between the gauge bosons quickly extend the momentum distribution towards high values, efficiently destroying the condensate after the onset of backreaction. For the inflationary scale $H = 10^8$ GeV, we find that 90% of the Higgs condensate has decayed after $n \sim 10$ oscillation cycles. This differs significantly from the Abelian case where, given the same coupling strengths, most of the condensate would persist after the resonance.

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)High Energy Physics::LatticeLattice field theoryFOS: Physical sciences01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - LatticeLattice (order)0103 physical sciences010306 general physicsSpecial unitary groupBosonCoupling constantPhysicsCondensed Matter::Quantum GasesGauge boson010308 nuclear & particles physicsHigh Energy Physics - Lattice (hep-lat)High Energy Physics::PhenomenologyAstronomy and AstrophysicsHigh Energy Physics - PhenomenologyHiggs bosonBack-reactionHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic Astrophysics
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Postinflationary vacuum instability and Higgs-inflaton couplings

2016

The Higgs-inflaton coupling plays an important role in the Higgs field dynamics in the early Universe. Even a tiny coupling generated at loop level can have a dramatic effect on the fate of the electroweak vacuum. Such Higgs-inflaton interaction is present both at the trilinear and quartic levels in realistic reheating models. In this work, we examine the Higgs dynamics during the preheating epoch, focusing on the effects of the parametric and tachyonic resonances. We use lattice simulations and other numerical tools in our studies. We find that the resonances can induce large fluctuations of the Higgs field which destabilize the electroweak vacuum. Our considerations thus provide an upper …

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)High Energy Physics::LatticePhysics beyond the Standard ModeleducationFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics114 Physical sciences01 natural sciencesUpper and lower boundsInstabilityGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)inflation Higgs0103 physical sciences010306 general physicsPhysicsCoupling010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyElectroweak interactionAstronomy and AstrophysicsInflatonHigh Energy Physics - PhenomenologyHiggs fieldHiggs bosonHigh Energy Physics::ExperimentAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Higgs-Inflaton Mixing and Vacuum Stability

2019

The quartic and trilinear Higgs field couplings to an additional real scalar are renormalizable, gauge and Lorentz invariant. Thus, on general grounds, one expects such couplings between the Higgs and an inflaton in quantum field theory. In particular, the (often omitted) trilinear coupling is motivated by the need for reheating the Universe after inflation, whereby the inflaton decays into the Standard Model (SM) particles. Such a coupling necessarily leads to the Higgs-inflaton mixing, which could stabilize the electroweak vacuum by increasing the Higgs self-coupling. We find that the inflationary constraints on the trilinear coupling are weak such that the Higgs-inflaton mixing up to ord…

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)cosmic inflationPhysics beyond the Standard ModelHigh Energy Physics::LatticeSTANDARD MODELFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsLorentz covariance01 natural sciences114 Physical sciencesHiggs inlationGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Higgs-inflaton couplings0103 physical sciences010306 general physicsquantum field theorykosminen inflaatioInflation (cosmology)Physicsta114010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::PhenomenologyBOSONInflatonlcsh:QC1-999Standard Model (mathematical formulation)Higgs fieldHigh Energy Physics - PhenomenologyHiggs bosonHigh Energy Physics::Experimentkvanttikenttäteorialcsh:PhysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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