English

The Observational Status of Simple Inflationary Models: an Update

High Energy Physics - Phenomenology 2016-04-28 v4 Cosmology and Nongalactic Astrophysics

Abstract

We provide an update on five relatively well motivated inflationary models in which the inflaton is a Standard Model singlet scalar field. These include i) the textbook quadratic and quartic potential models but with additional couplings of the inflaton to fermions and bosons, which enable reheating and also modify the naive predictions for the scalar spectral index nsn_s and rr, ii) models with Higgs and Coleman-Weinberg potentials, and finally iii) a quartic potential model with non-minimal coupling of the inflaton to gravity. For nsn_s values close to 0.96, as determined by the WMAP9 and Planck experiments, most of the considered models predict r0.02r\gtrsim0.02. The running of the scalar spectral index, quantified by dns/dlnk|\rm{d} n_s/\rm{d}\ln k|, is predicted in these models to be of order 10410^{-4}--10310^{-3}.

Keywords

Cite

@article{arxiv.1403.6403,
  title  = {The Observational Status of Simple Inflationary Models: an Update},
  author = {Nobuchika Okada and Vedat Nefer Şenoğuz and Qaisar Shafi},
  journal= {arXiv preprint arXiv:1403.6403},
  year   = {2016}
}

Comments

1+14 pages, 6 figures, 5 tables. v4: Title changed and manuscript revised taking into account Planck 2015 results