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Primordial black holes from CDM isocurvature perturbations
Phys. Rev. D 105, 103530 – Published 23 May, 2022
DOI: https://doi.org/10.1103/PhysRevD.105.103530
Abstract
We show that primordial black holes can be produced from the collapse of large isocurvature perturbations of the cold dark matter. We develop a novel procedure to compute the resulting black hole abundance by studying matched perturbations of matter-only universes, and we use our procedure to translate observational constraints on black hole abundances into model-independent constraints on cold dark matter isocurvature perturbations over a wide range of scales. The constraint on the typical amplitude of the primordial perturbations weakens slightly slower than linearly on small scales.
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