Can Standard Model Higgs Seed the Formation of Structures in Our Universe?
arXiv:1209.2277 · doi:10.1103/PhysRevD.87.043501
Abstract
We study the Standard Model Higgs field as a source for the primordial curvature perturbation, particularly in the curvaton and modulated reheating scenario. We conclude that the Higgs cannot play as a curvaton due to the small energy density when it decays, however the modulated reheating by Higgs can be a viable scenario. In the latter case, the non-Gaussianity is inevitably generated and strongly constrains the type of potential of inflaton field and Higgs-dependent interaction term. For the quadratic potential of the inflaton field with decay rate which non-linearly depends on the Higgs vacuum expectation value, the contribution of Higgs field to the primordial curvature perturbation must be less than 8%.
12 pages; version accepted for publication in Phys.Rev.D
References in corpus (21)
- 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
- The Standard Model Higgs boson as the inflaton
- Higgs inflation: consistency and generalisations
- Power-counting and the Validity of the Classical Approximation During Inflation
- Primordial Curvature Fluctuation and Its Non-Gaussianity in Models with Modulated Reheating
- Non-Gaussianity, Spectral Index and Tensor Modes in Mixed Inflaton and Curvaton Models
- Gravitational corrections to Standard Model vacuum decay
- A numerical study of non-gaussianity in the curvaton scenario
- Curvaton Dynamics and the Non-Linearity Parameters in Curvaton Model
- Large Non-Gaussianity Implication for Curvaton Scenario
- Correlated isocurvature perturbations from mixed inflaton-curvaton decay
- Generating the Curvature Perturbation at the End of Inflation in String Theory
- Scale-dependence of Non-Gaussianity in the Curvaton Model
- Hilltop Non-Gaussianity
- Higgs condensation as an unwanted curvaton
- Negative spectral index of in the axion-type curvaton model
- Non-Gaussianity and Gravitational Waves from Quadratic and Self-interacting Curvaton
- Multiple scalar particle decay and perturbation generation
- How the curvaton scenario, modulated reheating and an inhomogeneous end of inflation are related
- Non-Gaussianity and gravitational wave background in curvaton with a double well potential
Cited by in corpus (20)
- The First Three Seconds: a Review of Possible Expansion Histories of the Early Universe
- Higgs Scalaron Mixed Inflation
- Higgs Dynamics during Inflation
- Is a Higgs Vacuum Instability Fatal for High-Scale Inflation?
- Generation of the Higgs Condensate and Its Decay after Inflation
- A Cosmological Higgs Collider
- Bounce Inflation Cosmology with Standard Model Higgs Boson
- Non-Abelian dynamics in the resonant decay of the Higgs after inflation
- Lattice Calculation of the Decay of Primordial Higgs Condensate
- Planck constraints on Higgs modulated reheating of renormalization group improved inflation
- The Higgs field and early universe cosmology: a (brief) review
- Non-Gaussianities from the Standard Model Higgs
- Stochastic evolution of scalar fields with continuous symmetries during inflation
- Generic inference of inflation models by non-Gaussianity and primordial power spectrum reconstruction
- Inflation as an attractor in scalar cosmology
- Large Density Perturbations from Reheating to Standard Model particles due to the Dynamics of the Higgs Boson during Inflation
- Spectator Higgs, large-scale gauge fields and the non-minimal coupling to gravity
- Primordial non-Gaussianity from the Effects of the Standard Model Higgs during Reheating after Inflation
- Higgs-like spectator field as the origin of structure
- Reheating dynamics affects non-perturbative decay of spectator fields