Double-peaked inflation model: Scalar induced gravitational waves and primordial-black-hole suppression from primordial non-Gaussianity

A significant abundance of primordial black hole (PBH) dark matter can be produced by curvature perturbations with power spectrum Delta(2)(zeta) (k(peak)) similar to O(10(-2)) at small scales, associated with the generation of observable scalar induced gravitational waves (SIGWs). However, the primordial non-Gaussianity may play a non-negligible role, which is not usually considered. We propose two inflation models that predict double peaks of order O(10(-2)) in the power spectrum and study the effects of primordial non-Gaussianity on PBHs and SIGWs. This model is driven by a power-law potential, and has a noncanonical kinetic term whose coupling function admits two peaks. By field-redefinition, it can be recast into a canonical inflation model with two quasi-inflection points in the potential. We find that the PBH abundance will be altered saliently if non-Gaussianity parameter satisfies vertical bar f(NL)(k(peak), k(peak), k(peak))vertical bar Delta(2)(zeta) (k(peak))/(23 delta(3)(c))similar to O(10(-2)) Whether the PBH abundance is suppressed or enhanced depends on the f(NL) being positive or negative, respectively. In our model, non-Gaussianity parameter f(NL)(k(peak), k(peak), k(peak))similar to O(1) takes positive sign, thus PBH abundance is suppressed dramatically. On the contrary, SIGWs are insensitive to primordial non-Gaussianity and hardly affected, so they are still within the sensitivities of space-based GWs observatories and Square Kilometer Array.