Pebbles to Gems: Intermediate-mass black holes in the first star clusters
Benedetta Mestichelli, Manuel Arca Sedda, Marta Volonteri, Michela Mapelli, Stefano Torniamenti, Alessandro Lupi, Marica Branchesi, Shingo Hirano, Tomoaki Ishiyama, Ralf S. Klessen, Veronika Lipatova, Boyuan Liu
astro-ph.GA, astro-ph.CO
Submitted: 2026-07-03
Comments: 14 pages, 8 figures, 2 tables. Comments are welcome
Code: https://github.com/bmestichelli/RaccoonBinator
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Beyond Hierarchical Mergers: Accretion-Driven Origins of Massive, Highly Spinning Black Holes in Dense Star Clusters
- Growth of Light Seed Black Holes in the Early Universe
- Teen TITANS simulations -- I. Inefficient intermediate-mass black hole seeding via stellar collisions in young massive clusters
- Supermassive stars with embedded stellar black hole cores: dense assembling star clusters as faint multiple Little Red Dot systems
- FROST-CLUSTERS -- III. Metallicity-dependent intermediate mass black hole formation by runaway collisions in dense star clusters
- Star-Black Hole Interactions in Young Star Clusters
- The In Situ Growth of Stellar-mass "Light" Seed Black Holes in Nuclear Star Clusters
- Intermediate-mass black hole seeding in galactic nuclei from star cluster migration
- Direct N-body simulations of rotating and extremely massive Population III star clusters
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