Primordial blackhole formation: Exploring chaotic potential with a sharp step via the GLMS perspective
Rinsy Thomas, Jobil Thomas, Minu Joy

TL;DR
This paper investigates how a sharp step in a chaotic inflationary potential can lead to primordial black hole formation across multiple mass ranges, using the GLMS peak theory approximation and comparing it with the Press-Schechter formalism, aligning with observational constraints.
Contribution
It introduces a model with a sharp step in the potential that produces PBHs in four mass ranges and compares two different methods for calculating their abundance.
Findings
GLMS approximation predicts near-unity PBH abundance in small mass windows.
Press-Schechter formalism yields significantly lower PBH abundance.
Results are consistent with current observational constraints.
Abstract
A sharp step on a chaotic potential can enhance primordial curvature fluctuations on smaller scales to the to form primordial black holes (PBHs). The present study discusses an inflationary potential with a sharp step that results in the formation of PBHs in four distinct mass ranges. Also this inflationary model allows the separate consideration of observable parameters and on the CMB scale from the physics at small scales, where PBHs formation occur. In this work we computed the fractional abundance of PBHs () using the GLMS approximation of peak theory and also the Press-Schechter (PS) formalism. In the two typical mass windows, and , calculated using the GLMS approximation is nearly equal to 1 and that calculated via PS is of . In the other two mass windows and ,…
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