Revealing Four Subpopulations of Binary Black-Hole Mergers with the Fifth Gravitational-Wave Transient Catalog
Nir Guttman, Paul D. Lasky, Eric Thrane
astro-ph.HE
Submitted: 2026-07-24
Comments: 17 pages, 5 figures
Code: https://github.com/NirGutt/Four-Subpopulations-of-Binary-Black-Hole-Mergers
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- GWTC-5.0: An Introduction to Version 5.0 of the Gravitational-Wave Transient Catalog
- GWTC-5.0: Population Properties of Merging Compact Binaries
- GWTC-4.0: Population Properties of Merging Compact Binaries
- A subpopulation of low-mass, spinning black holes: signatures of dynamical assembly
- Characterizing Binary Black Hole Subpopulations in GWTC-4 with Binned Gaussian Processes: On the Origins of the $35M_{\odot}$ Peak
- Evidence for additional structure in the effective spin distribution hints at multiple formation pathways in GWTC-5.0
- Reversible-jump MCMC reveals binary black hole subpopulations with distinct redshift evolution
- Compactness Peaks and Subpopulations: Probing Stellar Physics and Formation Channels of Merging Binary Black Holes
- No model-independent evidence for a peak in binary black hole spin (mis)alignments
- Low-mass failed supernovae and the $10\,M_{\odot}$ peak in the merging black hole mass distribution
- GWPopulation: Hardware agnostic population inference for compact binaries and beyond
- Population of Binary Black Holes Inferred from One Hundred and Fifty Gravitational Wave Signals
- Joint population and strong-lensing inference for resolved gravitational-wave events probes the black-hole merger rate beyond the peak of star formation
- Emergent structure in the binary black hole mass distribution and implications for population-based cosmology
- A Thesaurus for Common Priors in Gravitational-Wave Astronomy
- Black hole mergers from dense star clusters with realistic binary populations
- When the black holes align: a subpopulation of aligned massive binary black holes observed via gravitational waves
- Transitions in the Mass-ratio and Spin Properties of Binary Black Holes in GWTC-5
- Distinct spin properties and astrophysical origin of low mass binary black holes in gravitational wave data
- Good things always come in 3s: trimodality in the binary black-hole chirp-mass distribution supports bimodal black-hole formation
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