skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Inflaton decay and reheating in nonminimal derivative coupling

Journal Article · · Journal of Cosmology and Astroparticle Physics
;  [1]
  1. Institute of Basic Science and Department of Computer Simulation, Inje University, Gimhae 621-749 (Korea, Republic of)

We investigate the inflaton decay and reheating period after the end of inflation in the non-minimal derivative coupling (NDC) model with chaotic potential. In general, this model is known to provide an enhanced slow-roll inflation caused by gravitationally enhanced friction. We find violent oscillations of Hubble parameter which induces oscillations of the sound speed squared, implying the Lagrangian instability of curvature perturbation ζ under the comoving gauge φ = 0. Also, it is shown that the curvature perturbation blows up at φ-dot = 0, leading to the breakdown of the comoving gauge at φ-dot = 0. Therefore, we use the Newtonian gauge to perform the perturbation analysis where the Newtonian potential is employed as a physical variable. The curvature perturbation is not considered as a physical variable which describes a relevant perturbation during reheating.

OSTI ID:
22679655
Journal Information:
Journal of Cosmology and Astroparticle Physics, Vol. 2016, Issue 07; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 1475-7516
Country of Publication:
United States
Language:
English

Similar Records

On the breakdown of the curvature perturbation ζ during reheating
Journal Article · Wed Apr 01 00:00:00 EDT 2015 · Journal of Cosmology and Astroparticle Physics · OSTI ID:22679655

Inflaton oscillations and post-inflationary reheating
Journal Article · Tue Apr 06 00:00:00 EDT 2021 · Journal of Cosmology and Astroparticle Physics · OSTI ID:22679655

More on loops in reheating: non-gaussianities and tensor power spectrum
Journal Article · Sun Jun 01 00:00:00 EDT 2014 · Journal of Cosmology and Astroparticle Physics · OSTI ID:22679655