paper

A Mid-Thirties Crisis: Dissecting the Properties of Gravitational Wave Sources Near the 35 Solar Mass Peak

arXiv:2507.01086 · doi:10.1088/1361-6382/ae1921

Abstract

One striking feature of binary black hole (BBH) mergers observed in the first decade of gravitational-wave astronomy is an excess of events with component masses around . Multiple formation channels have been proposed to explain this excess. To distinguish among these channels, it is essential to examine their predicted population-level distributions across additional parameters. In this work, we focus on BBH mergers near the peak and infer the population distributions of primary mass (), mass ratio (), effective spin (), and redshift (). We observe a gradual increase in the merger rate with , rising by a factor of from to a peak around , followed by a sharp, order-of-magnitude decline by . This population also shows a weak preference for equal-mass mergers and has a distribution skewed toward positive values, with a median of zero excluded at approximately confidence. We find no significant correlation in the peak population, suggesting that lower-mass systems () likely drive the anti-correlation observed in the full BBH merger catalog. The redshift evolution of the merger rate is consistent with the cosmic star formation rate. We compare our findings with predictions from a wide range of formation channels. We find that common variants of the pair-instability supernova scenario, as well as hierarchical mergers, are incompatible with the observed features of the population. Ultimately, none of the formation channels we consider can explain all or even most of the features observed in this population. The ''mid-thirties'' of black hole mergers are in crisis.

Accepted Version in Classical and Quantum Gravity Special Edition: Gravitational Wave Physics and Astrophysics Ten Years After GW150914. Codes are Publicly Available on GitHub: https://github.com/SoumendraRoy/35Msun_GWTC3. A Frozen Version of the Codes with Produced Data are Also Available on Zenodo: https://zenodo.org/records/15778343