When the black holes align: a subpopulation of aligned massive binary black holes observed via gravitational waves
astro-ph.HE
Submitted: 2026-06-22
Updated: 2026-09-14
Comments: 9 pages, 6 figures. Resubmitted after implementing referee's comments
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- GWTC-4.0: Population Properties of Merging Compact Binaries
- Evidence for additional structure in the effective spin distribution hints at multiple formation pathways in GWTC-5.0
- Evidence for Three Subpopulations of Merging Binary Black Holes at Different Primary Masses
- The first decade of gravitational-wave measurements of black hole spins
- Transitions in the Mass-ratio and Spin Properties of Binary Black Holes in GWTC-5
- Compactness Peaks and Subpopulations: Probing Stellar Physics and Formation Channels of Merging Binary Black Holes
- Evidence for mass-dependent spin subpopulations in GWTC-4
- Modern tidal interaction models for rapid binary population synthesis: II. Binary black hole formation, mergers, and spins
- Aligned Hierarchical Black Hole Mergers in Active-Galactic-Nuclei Disks Revealed by GWTC-4
- BBH-Genesis: Disentangling Binary Black Hole Formation Channels with GWTC-4
- Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset
- Reversible-jump MCMC reveals binary black hole subpopulations with distinct redshift evolution
- GWTC-5.0: Observations from the Second Part of the Fourth LIGO-Virgo-KAGRA Observing Run and Updates to the Gravitational-Wave Transient Catalog
- GWTC-5.0: Population Properties of Merging Compact Binaries
- Open Data from LIGO, Virgo, and KAGRA through the Second Part of the Fourth Observing Run
- AGN-driven BBH mergers: Black hole populations and hierarchical growth across the AGN parameter space
- Mass and effective spin distributions of binary black hole events: Evidence for a population of hierarchical black hole mergers in active galactic nuclei disks
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