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Inflation scenario via the Standard Model Higgs boson and LHC

Journal of Cosmology and Astroparticle Physics · 2008 · Vol. 2008(11) · pp. 021–021
A. O. BarvinskyAlexander Yu. KamenshchikAlexei A. Starobinsky

Abstract

We consider a quantum corrected inflation scenario driven by a generic GUT or Standard Model type particle model whose scalar field playing the role of an inflaton has a strong non-minimal coupling to gravity. We show that currently widely accepted bounds on the Higgs mass falsify the suggestion of the paper arXiv:0710.3755 (where the role of radiative corrections was underestimated) that the Standard Model Higgs boson can serve as the inflaton. However, if the Higgs mass could be raised to $\sim 230$ GeV, then the Standard Model could generate an inflationary scenario with the spectral index of the primordial perturbation spectrum $n_s\simeq 0.935$ (barely matching present observational data) and the very low tensor-to-scalar perturbation ratio $r\simeq 0.0006$.

Cosmology and Gravitation TheoriesBlack Holes and Theoretical PhysicsGalaxies: Formation, Evolution, PhenomenaPhysicsInflatonHiggs bosonParticle physicsSpectral indexStandard Model (mathematical formulation)Minimal Supersymmetric Standard ModelBosonInflation (cosmology)Physics beyond the Standard Model

Funding

  • Russian Foundation for Basic Research
  • Institut Périmètre de physique théorique
Citations
393
FWCI
13.48
field-weighted impact
References
42
Percentile
99%
vs. same field & year
Citations per year
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