Primordial spectra from sudden turning trajectory
- Mathematical Physics Laboratory, RIKEN Nishina Center, Saitama, 351–0198 (Japan)
- Department of Physics, Tokyo Institute of Technology, Tokyo, 152–8551 (Japan)
Effects of heavy fields on primordial spectra of curvature perturbations are discussed in inflationary models with a sudden turning trajectory. When heavy fields are excited after the sudden turn and oscillate around the bottom of the potential, the following two effects are generically induced: deformation of the inflationary background spacetime and conversion interactions between adiabatic and isocurvature perturbations, both of which can affect the primordial density perturbations. In this paper, we calculate primordial spectra in inflationary models with sudden turning potentials taking into account both of the two effects appropriately. We find that there are some non-trivial correlations between the two effects in the power spectrum and, as a consequence, the primordial scalar power spectrum has a peak around the scale exiting the horizon at the turn. Though both effects can induce parametric resonance amplifications, they are shown to be canceled out for the case with the canonical kinetic terms. The peak feature and the scale dependence of bispectra are also discussed.
- OSTI ID:
- 22369856
- Journal Information:
- Journal of Cosmology and Astroparticle Physics, Vol. 2013, Issue 12; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 1475-7516
- Country of Publication:
- United States
- Language:
- English
Similar Records
Oscillatory features in the curvature power spectrum after a sudden turn of the inflationary trajectory
CMB lensing forecasts for constraining the primordial perturbations: adding to the CMB temperature and polarization information