The Black Hole Accretion Code: adaptive mesh refinement and constrained transport
Hector Olivares, Oliver Porth, Yosuke Mizuno

TL;DR
This paper introduces the Black Hole Accretion Code (BHAC), a new GRMHD simulation tool that uses adaptive mesh refinement and constrained transport to efficiently model black hole accretion flows, aiding interpretation of upcoming VLBI observations.
Contribution
The paper presents modifications to integrate constrained transport with adaptive mesh refinement in BHAC, achieving high-precision magnetic field divergence control and improved computational efficiency.
Findings
Achieved machine precision in solenoidal magnetic field constraint.
Significant speedup in simulation performance.
Enhanced compatibility of constrained transport with AMR.
Abstract
With the forthcoming VLBI images of Sgr A* and M87, simulations of accretion flows onto black holes acquire a special importance to aid with the interpretation of the observations and to test the predictions of different accretion scenarios, including those coming from alternative theories of gravity. The Black Hole Accretion Code (BHAC) is a new multidimensional general-relativistic magnetohydrondynamics (GRMHD) module for the MPI-AMRVAC framework. It exploits its adaptive mesh refinement techniques (AMR) to solve the equations of ideal magnetohydrodynamics in arbitrary curved spacetimes with a significant speedup and saving in computational cost. In a previous work, this was shown using a Generalized Lagrange Multiplier (GLM) to enforce the solenoidal constraint of the magnetic field. While GLM is fully compatible with MPI-AMRVAC's AMR infrastructure, we found that simulations were…
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