We study slow roll single field inflationary scenario and the production of
non-thermal fermionic dark matter, together with standard model Higgs, during
reheating. For the inflationary scenario, we have considered two models of
polynomial potential - one is symmetric about the origin and another one is
not. We fix the coefficients of the potential from the current Cosmic Microwave
Background (CMB) data from Planck/Bicep. Next, we explore the allowed parameter
space on the coupling (yχ​) with inflaton and mass (mχ​) of dark
matter (DM) particles (χ) produced during reheating and satisfying CMB and
several other cosmological constraints.Comment: Prepared for Proceedings of XXV Bled Workshop "What comes beyond the
Standard models?