arXiv (OAI Expanded)
open access
Evidence for an accretion-driven subpopulation of black holes in GWTC-5.0
We report Bayesian evidence for a subpopulation of black holes, grown via accretion during the gaseous birth-stage of star clusters, in the cumulative GWTC-5.0 released by the LIGO-Virgo-KAGRA collaboration. This accretion channel predicts a saturating spin--mass relation, with low spins at low mass
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Evidence for an accretion-driven subpopulation of black holes in GWTC-5.0#793295
- Search for intermediate mass black hole binaries in the first and second observing runs of the Advanced LIGO and Virgo network#491773
- Search for intermediate mass black hole binaries in the first and second observing runs of the Advanced LIGO and Virgo network#370453
- When the black holes align: a subpopulation of aligned massive binary black holes observed via gravitational waves#1109085
- Binary Evolution Can Mimic the Pair-Instability Mass Gap in Black Hole Mergers#973137
Record · ID 789291
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive