Mechanism of primordial black holes production and secondary gravitational waves in $\alpha$-attractor Galileon inflationary scenario
Zeinab Teimoori, Kazem Rezazadeh, Mariwan Ahmed Rasheed, Kayoomars, Karami

TL;DR
This paper explores a novel inflationary model combining $ ext{alpha}$-attractor and Galileon theories to explain primordial black hole formation and secondary gravitational waves, matching observational constraints and predicting detectable signals.
Contribution
It introduces a new $ ext{alpha}$-attractor Galileon inflation model that successfully produces PBHs of various masses and predicts associated gravitational wave signals within observational sensitivity.
Findings
PBHs with masses around 10 solar masses, $10^{-5}$, and $10^{-13}$ solar masses are produced.
The model predicts secondary GWs with peak energy density $ imes 10^{-8}$, detectable by future GW detectors.
The GW spectrum follows a power-law relation with frequency in different ranges.
Abstract
We study the process of the Primordial Black Holes (PBHs) production in the novel framework, namely -attractor Galileon inflation (G-inflation) model. In our framework, we take the Galileon function as , where the part is motivated from the -attractor inflationary scenario in its original non-canonical frame, and it ensures for the model to be consistent with the Planck 2018 observations at the CMB scales. The part is invoked to enhance the curvature perturbations at some smaller scales which in turn gives rise to PBHs formation. By fine-tuning of the model parameters, we find three parameter sets which successfully produce a sufficiently large peak in the curvature power spectrum. We show that these parameter sets produce PBHs with masses , , and…
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