arXiv (All)
open access
Mass and spin properties of black-hole mergers reveal formation in triples
Deciphering the formation channels of the observed binary black hole mergers remains a central open problem in gravitational-wave astronomy. With hundreds of detections, the inferred distribution of masses and spins reveals a rich diversity which is difficult to reconcile with traditional formation
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
- Gravitational-wave signatures of primordial black hole clusters and the imprint of an early dense-core collapse#821278
- 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#1115835
- Stellar black hole binaries from two common envelope evolution phases in triple stellar systems#973235
- Probing Dark Matter with Gravitational Waves: Spin-Modulated Dephasing from Black Holes in Halos#612526
- Probing Dark Matter with Gravitational Waves: Spin-Modulated Dephasing from Black Holes in Halos#611049
Record · ID 1104577
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