A thesis that develops non-Gaussian PBH abundance computations, argues that broad power spectra are dominated by the broadest compaction profiles (threshold 2/5), and uses LVK and PTA data to constrain PBH models.
The curvature perturbation (and its derivative) grows because of the factor e−(3/2−ηII)N
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Cosmic Whispers of the Early Universe: Gravitational Waves and Dark Matter from Primordial Black Holes
A thesis that develops non-Gaussian PBH abundance computations, argues that broad power spectra are dominated by the broadest compaction profiles (threshold 2/5), and uses LVK and PTA data to constrain PBH models.