Outliers in the LIGO Black Hole Mass Function from Coagulation in Dense Clusters
Jordan Flitter, Julian B. Mu\~noz, Ely D. Kovetz

TL;DR
This paper investigates the origin of outlier black hole mergers observed by LIGO, proposing a hierarchical coagulation model in dense clusters to explain their mass properties and predict future observational constraints.
Contribution
It introduces a coagulation-based model for black hole mass evolution in clusters, linking it to LIGO observations and forecasting constraints from future data.
Findings
Hierarchical mergers can produce outlier masses observed by LIGO.
The model predicts merger distributions consistent with O3a data.
Future O5 data can distinguish between coagulation and static channels.
Abstract
The advanced LIGO O3a run catalog has been recently published, and it includes several events with unexpected mass properties, including mergers with individual masses in the lower and upper mass gaps, as well as mergers with unusually small mass ratios between the binary components. Here we entertain the possibility that these outliers are the outcome of hierarchical mergers of black holes or neutron stars in the dense environments of globular clusters. We use the coagulation equation to study the evolution of the black hole mass function within a typical cluster. Our prescription allows us to monitor how various global quantities change with time, such as the total mass and number of compact objects in the cluster, its overall merger rate, and the probability to form intermediate-mass black holes via a runaway process. By accounting for the LIGO observational bias, we predict the…
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