Warm Inflation with the Standard Model
Kim V. Berghaus, Marco Drewes, Sebastian Zell
Abstract
We show for the first time that warm inflation is feasible with standard model (SM) gauge interactions alone. Our model consists of a minimal extension of the SM by a single scalar inflaton field with an axionlike coupling to gluons and a monomial potential. The effects of light fermions, which were previously argued to render warm inflation with the SM impossible, are alleviated by Hubble dilution of their chiral chemical potentials. Our model features only one adjustable combination of parameters and accommodates all inflationary observables. We briefly discuss implications for axion experiments, dark matter, and the strong CP problem.
Topics & Concepts
InflatonPhysicsInflation (cosmology)AxionStandard Model (mathematical formulation)Particle physicsHubble's lawGauge (firearms)Theoretical physicsCoupling (piping)Scalar fieldDark matterScalar (mathematics)Higgs bosonMonomialMinimal Supersymmetric Standard ModelGluonPhysics beyond the Standard ModelCosmologyGauge theoryCosmic background radiationUniverseMassless particleSlow rollMinimal couplingQuantum electrodynamicsHiggs fieldDilutionCosmic microwave backgroundStatistical physicsInflationary epochCoupling parameterCosmology and Gravitation TheoriesDark Matter and Cosmic PhenomenaClimate variability and models