2014/03/31 by Nobuchika Okada, V. N. Şenoğuz, Vedat Nefer Şenoğuz +1 · 47 citations
Mathematics · Physics and Astronomy · #Boson #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Higgs boson #Inflation (cosmology) #Inflaton #Mathematical physics #Mathematics #Particle physics #Particle physics theoretical and experimental studies #Physics #Planck #Quantum mechanics #Quartic function #Scalar (mathematics) #Scalar field #Spectral index #Spectral line #Theoretical physics #astro-ph.CO #hep-ph
paper · pdf · doi:10.3906/fiz-1505-7
published in TURKISH JOURNAL OF PHYSICS 40, 150-162 (Scientific and Technological Research Council of Turkey (TUBITAK)) · 1+14 pages, 6 figures, 5 tables. v4: Title changed and manuscript revised taking into account Planck 2015 results
arxiv created 2015/05/13 · openalex publication_date 2016/01/01 · arxiv updated 2016/04/28 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
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 ns and r, ii) models with Higgs and Coleman-Weinberg potentials, and finally iii) a quartic potential model with nonminimal coupling of the inflaton to gravity. For ns values close to 0.96, as determined by the WMAP9 and Planck experiments, most of the considered models predict r\gtrsim0.02. The running of the scalar spectral index, quantified by \ud ns/\udln k , is predicted in these models to be of order 10-4-10-3.