K-Essence Induced by Derivative Couplings of the Inflaton
arXiv:2303.09880 · doi:10.1103/PhysRevD.107.103533
Abstract
We consider two models which couple derivatives of the inflaton to ordinary matter, both to fermions and to scalars. Such couplings induce changes to the inflaton kinetic energy, analogous to the cosmological Coleman-Weinberg potentials which come from nonderivative couplings. Our purpose is to investigate whether these quantum-induced K-Essence models can provide efficient reheating without affecting the observational constraints on primordial inflation. Our numerical studies show that it is difficult to preserve both properties.
27 pages, 19 figures, uses LaTeX2e, Appendix is added
References in corpus (6)
- BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season
- Improved limits on the tensor-to-scalar ratio using BICEP and Planck
- Dark Energy: the equation of state description versus scalar-tensor or modified gravity
- Leading Log Solution for Inflationary Yukawa
- Reheating temperature from the CMB
- Inflaton Effective Potential from Photons for General