PBHs and GWs from ${\mathbb{T}}^2$-inflation and NANOGrav 15-year data

Abstract

In this paper, we propose a novel mechanism in ${\mathbb{T}}^2$-inflation to enhance the power spectrum large enough to seed primordial black holes (PBHs) formation. To accomplish this, we consider the coupling function between the inflaton field and ${\mathbb{T}}^2=T_{\mu \nu }{T}^{\mu \nu }$ term. PBHs formed within this scenario can contribute partially or entirely to dark matter (DM) abundance. Furthermore, the amplification in the scalar power spectrum will concurrently produce significant scalar-induced gravitational waves (SIGWs) as a second-order effect. In addition, the energy spectrum associated with SIGWs can be compatible with the recent NANOGrav 15-year stochastic gravitational wave detection and fall into the sensitivity range of other forthcoming GW observatories.

8 pages, 7 figures, and one table, references added, accepted by JCAP