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Primordial black holes from CDM isocurvature perturbations

Samuel Passaglia1,* and Misao Sasaki1,2,3,†

  • 1Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study (UTIAS), The University of Tokyo, Chiba 277-8583, Japan
  • 2Center for Gravitational Physics, Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-8502, Japan
  • 3Leung Center for Cosmology and Particle Astrophysics, National Taiwan University, Taipei 10617, Taiwan

  • *samuel.passaglia@ipmu.jp
  • misao.sasaki@ipmu.jp

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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