Universal radial scaling of large-scale black hole accretion for magnetically arrested and rocking accretion disks

We thank Martijn Oei, Ioannis Liodakis, Anthony Readhead, and Eliot Quataert for helpful discussions. A. T. was supported by NSF Grants No. AST-2009884, No. AST-2107839, No. AST-1815304, No. AST-1911080, No. AST-2206471, No. AST-2407475, and No. OAC-2031997, and by NASA Grants No. 80NSSC22K0031, No. 80NSSC22K0799, No. 80NSSC18K0565, and No. 80NSSC21K1746. Support for this work was provided by the National Aeronautics and Space Administration through Chandra Award No. TM1-22005X issued by the Chandra X-ray Center, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of the National Aeronautics Space Administration under Contract No. NAS8-03060. The authors acknowledge the Texas Advanced Computing Center (TACC) at The University of Texas at Austin for providing HPC and visualization resources that have contributed to the research results reported within this paper via the LRAC allocation AST20011 [75]. This research used resources from the Oak Ridge Leadership Computing Facility, which is a DOE Office of Science User Facility supported under Contract No. DE-AC05-00OR22725. An award of computer time was provided by the ASCR Leadership Computing Challenge (ALCC), Innovative and Novel Computational Impact on Theory and Experiment (INCITE), and the OLCF Director’s Discretionary Allocation programs under award PHY129. This research used resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231 using NERSC award ALCC-ERCAP0022634. This research used resources of the National Energy Research Scientific Computing Center (NERSC), a U.S. Department of Energy Office of Science User Facility located at Lawrence Berkeley National Laboratory, operated under Contract No. DE-AC02-05CH11231 using NERSC ERCAP Award No. m2401 for 2022–2025. E. R. M. acknowledges support through the Oak Ridge Leadership Computing Facility at the Oak Ridge National Laboratory, which is supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC05-00OR22725, and the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231, and NERSC Award No. NP-ERCAP0028480. B. R. acknowledges support by the Natural Sciences & Engineering Research Council of Canada (NSERC), the Canadian Space Agency (23JWGO2A01), and by a grant from the Simons Foundation (Grant No. MP-SCMPS-00001470). B. R. acknowledges a guest researcher position at the Flatiron Institute, supported by the Simons Foundation.

The data that support the findings of this article are not publicly available. The data are available from the authors upon reasonable request.