Curvaton Decay by Resonant Production of the Standard Model Higgs
arXiv:1211.5028 · doi:10.1088/1475-7516/2013/01/040
Abstract
We investigate in detail a model where the curvaton is coupled to the Standard Model higgs. Parametric resonance might be expected to cause a fast decay of the curvaton, so that it would not have time to build up the curvature perturbation. However, we show that this is not the case, and that the resonant decay of the curvaton may be delayed even down to electroweak symmetry breaking. This delay is due to the coupling of the higgs to the thermal background, which is formed by the Standard Model degrees of freedom created from the inflaton decay. We establish the occurrence of the delay by considering the curvaton evolution and the structure of the higgs resonances. We then provide analytical expressions for the delay time, and for the subsequent resonant production of the higgs, which ultimately leads to the curvaton effective decay width. Contrary to expectations, it is possible to obtain the observed curvature perturbation for values of the curvaton-higgs coupling as large as 0.1. Our calculations also apply in the general case of curvaton decay into any non Standard Model species coupled to the thermal background.
arXiv comment39 pages, 2 figures. v2 matches published version (one reference added)
References in corpus (30)
- Observation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC
- Observation of a new boson at a mass of 125 GeV with the CMS experiment at the LHC
- Towards the Theory of Reheating After Inflation
- Reheating after Inflation
- Generating the curvature perturbation without an inflaton
- Universe Reheating after Inflation
- Adiabatic CMB perturbations in pre-big bang string cosmology
- Effects of Cosmological Moduli Fields on Cosmic Microwave Background
- Structure of Resonance in Preheating after Inflation
- On initial conditions for the Hot Big Bang
- Preheating in the Standard Model with the Higgs-Inflaton coupled to gravity
- Theory and Numerics of Gravitational Waves from Preheating after Inflation
- Particle physics models of inflation and curvaton scenarios
- Gauge invariant MSSM inflaton
- A Gravitational Wave Background from Reheating after Hybrid Inflation
- Gravitational Wave Production At The End Of Inflation
- MSSM flat direction inflation: slow roll, stability, fine tunning and reheating
- Gravitational Waves from Abelian Gauge Fields and Cosmic Strings at Preheating
- Dynamics of oscillating scalar field in thermal environment
- Preheating and the non-gaussianity of the curvature perturbation
- On the Transverse-Traceless Projection in Lattice Simulations of Gravitational Wave Production
- Non-perturbative production of matter and rapid thermalization after MSSM inflation
- Non-Gaussianity from resonant curvaton decay
- Parametric Decay of the Curvaton
- Preheating the Universe from the Standard Model Higgs
- Stochastic Background of Gravitational Waves from Fermions
- Quantum Corrections to Inflaton and Curvaton Dynamics
- Electrically charged curvaton
- Curvaton model completed
- Curvaton preheating revisited
Cited by in corpus (26)
- Cosmological Backgrounds of Gravitational Waves
- Update on scalar singlet dark matter
- Electroweak Vacuum Stability in light of BICEP2
- The art of simulating the early Universe -- Part I
- Gravitational wave production from preheating: parameter dependence
- Generation of the Higgs Condensate and Its Decay after Inflation
- The Decay of the Standard Model Higgs after Inflation
- Parametric Resonance in the Early Universe - A Fitting Analysis
- On the Anisotropy of the Gravitational Wave Background from Massless Preheating
- Stochastic Background of Gravitational Waves from Fermions -- Theory and Applications
- Fate of Symmetric Scalar Field
- Non-Abelian dynamics in the resonant decay of the Higgs after inflation
- On finite density effects on cosmic reheating and moduli decay and implications for Dark Matter production
- Scalar Trapping and Saxion Cosmology
- The Higgs field and early universe cosmology: a (brief) review
- Non-minimally coupled curvaton
- The minimal curvaton-higgs model
- Curvaton Dynamics Revisited
- Sensitivity of gravitational waves from preheating to a scalar field's interactions
- Present and future of CosmoLattice
- Thermal blocking of preheating
- The running curvaton
- Preheating with higher dimensional interaction
- Reheating dynamics affects non-perturbative decay of spectator fields
- Quantifying the 'naturalness' of the curvaton model
- Quenching preheating by light fields