Primordial black holes and gravitational waves from parametric amplification of curvature perturbations
Rong-Gen Cai, Zong-Kuan Guo, Jing Liu, Lang Liu, Xing-Yu Yang

TL;DR
This paper proposes a new inflationary mechanism involving parametric resonance that amplifies curvature perturbations, leading to primordial black holes and gravitational waves detectable by current observatories.
Contribution
It introduces a novel parametric resonance process in single-field inflation models that can produce observable primordial black holes and gravitational waves.
Findings
Primordial black holes could account for all or part of dark matter.
Generated gravitational waves are within detectable frequency ranges.
The model's parameters determine black hole mass and gravitational wave frequency.
Abstract
We investigate a new mechanism to create large curvature perturbations on small scales due to parameter resonance in a single-field inflationary model with a small periodic structure upon the potential. After reentering the horizon, the amplified curvature perturbations can lead to observable primordial black holes as well as stochastic gravitational waves. The mass of primordial black holes and frequency of the induced gravitational waves depend on the model parameters. The resulted primordial black hole could constitute all dark matter or a fraction of dark matter in the universe, and corresponding stochastic gravitational waves fall in the frequency band measurable for the pulsar timing array and the space-based gravitational wave detectors.
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