Hybrid Inflation Revisited in Light of WMAP5
arXiv:0901.4345 · doi:10.1103/PhysRevD.79.103503
Abstract
We study the effects of including one-loop radiative corrections in a non-supersymmetric hybrid inflationary model. These corrections can arise from Yukawa couplings between the inflaton and right-handed neutrinos, and induce a maximum in the potential which admits hilltop-type solutions in addition to the standard hybrid solutions. We obtain a red-tilted spectral index , consistent with WMAP5 data, for sub-Planckian values of the field. This is in contrast to the tree level hybrid analysis, in which a red-tilted spectrum is achieved only for trans-Planckian values of the field. Successful reheating is obtained at the end of the inflationary phase via conversion of the inflaton and waterfall fields into right-handed neutrinos, whose subsequent decay can explain the observed baryon asymmetry via leptogenesis.
18 pages (double spaced), including 6 figures and 1 table (v1); 13 pages (single spaced), added 3 references to Ref. [14] and modified placement of table and some figures (v2)
References in corpus (9)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Inflation after WMAP3: Confronting the Slow-Roll and Exact Power Spectra with CMB Data
- Supersymmetric Hybrid Inflation with Non-Minimal Kahler potential
- More hilltop inflation models
- Supersymmetric And Smooth Hybrid Inflation In The Light Of WMAP3
- Testing String Theory with CMB
- Anatomy of F_D-Term Hybrid Inflation
- Chaotic inflation, radiative corrections and precision cosmology
- Realistic Hybrid Inflation in 5D Orbifold SO(10) GUT