Horizon-scale intensity and polarization images of rotating Konoplya-Zhidenko black holes with thick accretion flows

arXiv:2607.01017 · gr-qc, astro-ph.HE · Submitted 2026-07-01 · Read on arXiv

gr-qc, astro-ph.HE

Submitted: 2026-07-01

Updated: 2026-10-03

Comments: 22 pages, 8 figures

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

Terminology

• Event Horizon Telescope — 7× in this paper
• Adam — 6× in this paper · explained in 2 episodes
• Accretion Flows — 5× in this paper · explained in 1 episode
• Gravitational Lensing — 5× in this paper · explained in 2 episodes
• Calibration — 1× in this paper · explained in 7 episodes
• In Boyer-Lindquist — 1× in this paper
• Quintessence — 1× in this paper · explained in 2 episodes

Sources

• Advection-Dominated Accretion: A Self-Similar Solution
• Semi-analytic studies of accretion disk and magnetic field geometry in M87*
• Distinguishing Black Holes and Neutron Stars via Optical Images Illuminated by Thick Accretion Disks
• Observational features of the Bardeen-boson star with thin disk accretion
• Non-thermal Synchrotron Emission and Polarization Signatures during Black Hole Flux Eruptions

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