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Primordial black holes and secondary gravitational waves from natural inflation

Published 7 Dec 2020 in gr-qc | (2012.03856v3)

Abstract: The production of primordial black hole (PBH) dark matter (DM) and the generation of scalar induced secondary gravitational waves by using the enhancement mechanism with a peak function in the non-canonical kinetic term in natural inflation is discussed. We show explicitly that the power spectrum for the primordial curvature perturbation can be enhanced at $10{12}$ Mpc${-1}$, $10{8}$ Mpc${-1}$ and $10{5}$ Mpc${-1}$ by adjusting the model parameters. With the enhanced primordial curvature perturbations, we show the production of PBH DM with peak masses around $10{-13}\ M_{\odot}$, the Earth's mass and the stellar mass, and the generation of scalar induced gravitational waves (SIGWs) with peak frequencies around mHz, $10{-6}$ Hz and nHz, respectively. The PBHs with the mass scale $10{-13}\ M_{\odot}$ can make up almost all the DM and the associated SIGWs is testable by spaced based gravitational wave observatory.

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