Accretion of multipolar massive complex scalar field packets by a Schwarzschild black hole

arXiv:2607.18920 · gr-qc, astro-ph.GA · Submitted 2026-07-21 · Read on arXiv

Flavio Rosales-Infante, Ivan Alvarez-Rios, Francisco S. Guzman

gr-qc, astro-ph.GA

Submitted: 2026-07-21

Comments: 19 pages, 11 figures. Submitted to Phys. Rev. D

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

Terminology

• Initial Data — 6× in this paper · explained in 2 episodes
• Core — 5× in this paper · explained in 2 episodes
• Consistency — 4× in this paper · explained in 3 episodes
• Absorption Cross Section — 3× in this paper · explained in 1 episode
• Degeneracy — 2× in this paper · explained in 3 episodes
• Accuracy — 1× in this paper · explained in 1 episode
• Quintessence — 1× in this paper · explained in 2 episodes
• Trace — 1× in this paper · explained in 2 episodes
• Verification — 1× in this paper · explained in 2 episodes

Sources

• Universailty of Low Energy Absorption Cross-sections for Black Holes
• Absorption of a massive scalar field by a charged black hole
• Scalar absorption by charged rotating black holes
• Scalar absorption: Black holes versus wormholes
• Are black holes a serious threat to scalar field dark matter models?
• Horizon growth of supermassive black hole seeds fed with collisional dark matter
• Quasistationary solutions of scalar fields around accreting black holes
• First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole
• Schwarzschild black holes can wear scalar wigs
• Schwarzschild scalar wigs: spectral analysis and late time behavior
• Black Holes as Condensation Points of Fuzzy Dark Matter Cores

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