Dynamical pairing in gravitational wave populations
astro-ph.HE
Submitted: 2026-10-07
Updated: 2026-10-07
Comments: 20 pages, 11 figures. Comments are welcomed
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Sources
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- GWTC-5.0: Methods for Identifying and Characterizing Gravitational-wave Transients
- Population Properties of Compact Objects from the Second LIGO-Virgo Gravitational-Wave Transient Catalog
- Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo
- GWTC-5.0: Population Properties of Merging Compact Binaries
- The population of merging compact binaries inferred using gravitational waves through GWTC-3
- A Star Cluster Population of High Mass Black Hole Mergers in Gravitational Wave Data
- Binary Black Hole Phase Space Discovers the Signature of Pair Instability Supernovae Mass Gap
- Gravitational-wave constraints on the pair-instability mass gap and nuclear burning in massive stars
- Cosmic Cousins: Identification of a Subpopulation of Binary Black Holes Consistent with Isolated Binary Evolution
- Seeking Spinning Subpopulations of Black Hole Binaries via Iterative Density Estimation
- Potential Subpopulations and Assembling Tendency of the Merging Black Holes
- The binary black hole spin distribution likely broadens with redshift
- Picky Partners: The Pairing of Component Masses in Binary Black Hole Mergers
- Who Ordered That? Unequal-Mass Binary Black Hole Mergers Have Larger Effective Spins
- Coalescing black hole binaries from globular clusters: mass distributions and comparison to gravitational wave data from GWTC-3
- Two of a Kind: Comparing big and small black holes in binaries with gravitational waves
- Hints of spin-magnitude correlations and a rapidly spinning subpopulation of binary black holes
- Searching for binary black hole sub-populations in gravitational wave data using binned Gaussian processes
- Phase Space of Binary Black Holes from Gravitational Wave Observations to Unveil its Formation History
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