Black hole spin-mass correlation and vector resonant relaxation in gaseous star clusters: the origin of GW231123?

arXiv:2607.17869 · astro-ph.HE, astro-ph.GA · Submitted 2026-07-20 · Read on arXiv

Zacharias Roupas

astro-ph.HE, astro-ph.GA

Submitted: 2026-07-20

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Core — 6× in this paper · explained in 2 episodes
• Metallicity — 6× in this paper · explained in 3 episodes
• Alignment — 4× in this paper · explained in 1 episode
• Consistency — 3× in this paper · explained in 3 episodes
• Self-consistency — 3× in this paper · explained in 2 episodes
• James Webb Space Telescope — 1× in this paper
• Phase Transitions — 1× in this paper · explained in 2 episodes
• Trace — 1× in this paper · explained in 2 episodes

Sources

• Accretion-disk formation around orbiting stellar black holes in gaseous star clusters

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