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astro-ph.HE2024
Toward 2D Dynamo Models Calibrated by Global 3D Relativistic Accretion Disk Simulations
Matthew D. Duez, Courtney L. Cadenhead, Zachariah B. Etienne +2
Two-dimensional models assuming axisymmetry are an economical way to explore the long-term evolution of black hole accretion disks, but they are only realistic if the feedback of t…
astro-ph.HE2024
A Parameter Study of the Electromagnetic Signatures of an Analytical Mini-Disk Model for Supermassive Binary Black Hole Systems
Kaitlyn Porter, Scott C. Noble, Eduardo M. Gutierrez +4
Supermassive black holes (SMBHs) are thought to be located at the centers of most galactic nuclei. When galaxies merge they form supermassive black hole binary (SMBHB) systems and…