Primordial black holes (PBH) can efficiently form black hole binaries in the early universe. We update the resulting constraints on PBH abundance using data from the third observational run (O3) of LIGO-Virgo-KAGRA. To capture a wide range of PBH scenarios, we consider a variety of mass functions, including critical collapse in the QCD epoch in the presence of non-Gaussianities. Applying hierarchical Bayesian analysis to a population binaries consisting of primordial and astrophysical black holes, we find that, in every scenario, the PBHs can make up at most fPBH≲10−3 of dark matter in the mass range 1−200M⊙. The shape and strength of the constraints are insensitive to the type of non-Gaussianities, the modifications to the mass function during the QCD epoch, or the modelling of the astrophysical PBH population.
@article{arxiv.2405.05732,
title = {Constraints on primordial black holes from LIGO-Virgo-KAGRA O3 events},
author = {M. Andrés-Carcasona and A. J. Iovino and V. Vaskonen and H. Veermäe and M. Martínez and O. Pujolàs and Ll. M. Mir},
journal= {arXiv preprint arXiv:2405.05732},
year = {2024}
}