Primordial blackholes and gravitational waves for an inflection-point model of inflation

In this article we provide a new closed relationship between cosmic abundance of primordial gravitational waves and primordial blackholes that originated from initial inflationary perturbations for inflection-point   models of inflation where inflation occurs below the Planck scale. The current Planck constraint on tensor-to-scalar ratio, running of the spectral tilt, and from the abundance of dark matter content in the universe, we can deduce a strict bound on the current abundance of primordial blackholes to be within a range, 9.99712×10−3<ΩPBHh2<9.99736×10−39.99712×10−3<ΩPBHh2<9.99736×10−3.