The astro-primordial black hole merger rates: a reappraisal
Konstantinos Kritos, Valerio De Luca, Gabriele Franciolini, Alex Kehagias, Antonio Riotto
Abstract
Abstract Mainly motivated by the recent GW190521 mass gap event which we take as a benchmark point, we critically assess if binaries made of a primordial black hole and a black hole of astrophysical origin may form, merge in stellar clusters and reproduce the LIGO/Virgo detection rate. While two previously studied mechanisms — the direct capture and the three body induced — seem to be inefficient, we propose a new “catalysis” channel based on the idea that a subsequent chain of single-binary and binary-binary exchanges may lead to the formation of a high mass binary pairs and show that it may explain the recent GW190521 event if the local overdensity of primordial black holes in the globular cluster is larger than a few.