The power spectrum on small scales: robust constraints and comparing PBH methodologies

Andrew David Gow*, Christian T. Byrnes, Philippa S. Cole, Sam Young

*Corresponding author for this work

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Abstract

We compare primordial black hole (PBH) constraints on the power spectrum and mass distributions using the traditional Press Schechter formalism, peaks theory, and a recently developed version of peaks theory relevant to PBHs. We show that, provided the PBH formation criteria and the power spectrum smoothing are treated consistently, the constraints only vary by ∼10% between methods (a difference that will become increasingly important with better data). Our robust constraints from PBHs take into account the effects of critical collapse, the non-linear relation between ζ and δ, and the shift from the PBH mass to the power spectrum peak scale. We show that these constraints are remarkably similar to the pulsar timing array (PTA) constraints impacting the black hole masses detected by LIGO and Virgo, but that the μ-distortion constraints rule out supermassive black hole (SMBH) formation and potentially even the much lighter mass range of ∼(1–100) M that LIGO/Virgo probes.
Original languageEnglish
Article number002
Number of pages31
JournalJournal of Cosmology and Astroparticle Physics
Volume2021
Issue number02
DOIs
Publication statusPublished - 2 Feb 2021
Externally publishedYes

Keywords

  • Primordial black holes
  • Physics of the early universe
  • Cosmological perturbation theory
  • UKRI
  • STFC
  • ST/T000473/1
  • ST/N504452/1

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