Fitting power spectrum of scalar perturbations for primordial black hole production during inflation

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Fitting power spectrum of scalar perturbations for primordial black hole production during inflation	514 KB	Adobe Acrobat PDF	Read	Download
DOI Доступ к ресурсу на сайте издателя			10.3390/astronomy2010005

Title: Fitting power spectrum of scalar perturbations for primordial black hole production during inflation
Creator: Frolovsky, Daniel
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Ketov, Sergei V.
Date: 2023
DOI: 10.3390/astronomy2010005
Description: A simple phenomenological fit for the power spectrum of scalar (curvature) perturbations during inflation is proposed to analytically describe slow roll of inflaton and formation of primordial black holes (PBH) in the early universe, in the framework of single-field models. The fit is given by a sum of the power spectrum of slow-roll inflation, needed for a viable description of the cosmic microwave background (CMB) radiation in agreement with Planck/BICEP/Keck measurements, and the log-normal (Gaussian) fit for the power spectrum enhancement (peak) needed for efficient PBH production, in the leading (model-independent) approximation. The T-type α-attractor models are used to get the simple CMB power spectrum depending upon the e-folds as the running variable. The location and height of the peak are chosen to yield the PBH masses in the asteroid-size window allowed for the whole (current) dark matter. We find the restrictions on the peak width