Relativistic Common-envelope Dynamics of a Stellar-mass Black Hole II: Kerr Black Hole

arXiv:2607.07462 · astro-ph.HE, gr-qc · Submitted 2026-07-08 · Read on arXiv

Alejandro Cruz-Osorio, Fabio D. Lora-Clavijo

astro-ph.HE, gr-qc

Submitted: 2026-07-08

Comments: 9 pages, 3 figures, 2 tables. Accepted for publication in MNRAS

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

Terminology

• Core — 4× in this paper · explained in 2 episodes
• Accuracy — 1× in this paper · explained in 1 episode
• Angular Momentum Transport — 1× in this paper · explained in 3 episodes
• Calibration — 1× in this paper · explained in 7 episodes
• Conservation Laws — 1× in this paper · explained in 3 episodes
• Consistency — 1× in this paper · explained in 3 episodes
• Initial Data — 1× in this paper · explained in 2 episodes
• Population Synthesis — 1× in this paper · explained in 2 episodes

Sources

• The shocks during the accretion of an ultrarelativistic supersonic gas onto a rotating black hole
• Jet Formation in 3D GRMHD Simulations of Bondi-Hoyle-Lyttleton Accretion
• General relativistic magnetized Bondi-Hoyle-Lyttleton accretion with a spin-field misalignment: Jet nutation, polarity reversals, and Magnus drag

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