Binary black holes gone MAD: Magnetically arrested minidisks around nonspinning black holes
arXiv:2509.18254 · doi:10.1103/g98b-m8m1
Abstract
We demonstrate the formation of magnetically arrested minidisks (MAM) around equal-mass, nonspinning binary black holes with magnetohydrodynamic simulations of circumbinary disk accretion in full 3+1 general relativity. The initial separation of allows the black holes to host large minidisks that suppress the total rest-mass accretion rate variability, which is modulated primarily at . Each black hole horizon saturates with dimensionless magnetic flux . Magnetic reconnection near the horizons drives recurrent eruptions which are expected to drive flaring in the infrared and X-ray bands. Our results establish MAMs as a new outcome of circumbinary disk accretion, and a promising source of novel electromagnetic counterparts to gravitational waves from binary black holes.
12 pages, 3 figures. Supplemental movie: https://youtube.com/shorts/89F_4GaaXo8?feature=share
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