Not all spins of black-hole binaries formed in clusters are isotropic and not all spins of black-hole binaries formed in isolation are aligned
astro-ph.HE, gr-qc
Submitted: 2026-09-25
Updated: 2026-09-25
Terminology
Sources
- GWTC-5.0: Population Properties of Merging Compact Binaries
- Merging stellar-mass binary black holes
- Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures
- Constraining the fraction of binary black holes formed in isolation and young star clusters with gravitational-wave data
- One Channel to Rule Them All? Constraining the Origins of Binary Black Holes using Multiple Formation Pathways
- Black Hole Formation in Failing Core-Collapse Supernovae
- Most Black Holes are Born Very Slowly Rotating
- Illuminating Black Hole Binary Formation Channels with Spins in Advanced LIGO
- Hierarchical analysis of gravitational-wave measurements of binary black hole spin-orbit misalignments
- Use of gravitational waves to probe the formation channels of compact binaries
- Determining the population properties of spinning black holes
- Spin orientations of merging black holes formed from the evolution of stellar binaries
- Dropping Anchor: Understanding the Populations of Binary Black Holes with Random and Aligned Spin Orientations
- Spin-Orbit Misalignment in Close Binaries with Two Compact Objects
- The origin of spin in binary black holes: Predicting the distributions of the main observables of Advanced LIGO
- Flipping spins in mass transferring binaries and origin of spin-orbit misalignment in binary black holes
- A Diverse Distribution of Black Hole Spins from Stable Mass Transfer
- Resonant-plane locking and spin alignment in stellar-mass black-hole binaries: a diagnostic of compact-binary formation
- Pathways for producing binary black holes with large misaligned spins in the isolated formation channel
- Revising the Spin and Kick Connection in Isolated Binary Black Holes
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