Papers › Iharm3D: Vectorized General Relativistic Magnetohydrodynamics
Iharm3D: Vectorized General Relativistic Magnetohydrodynamics
Cora Prather, George N. Wong, Vedant Dhruv, Benjamin R. Ryan, Joshua C. Dolence, Sean M. Ressler, Charles F. Gammie
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Iharm3D is an open-source C code for simulating black hole accretion systems in arbitrary stationary spacetimes using ideal general-relativistic magnetohydrodynamics (GRMHD). It is an implementation of the HARM ("High Accuracy Relativistic Magnetohydrodynamics") algorithm outlined in Gammie et al. (2003) with updates as outlined in McKinney & Gammie (2004) and Noble et al. (2006). The code is most directly derived from Ryan et al. (2015) but with radiative transfer portions removed. HARM is a conservative finite-volume scheme for solving the equations of ideal GRMHD, a hyperbolic system of partial differential equations, on a logically Cartesian mesh in arbitrary coordinates.
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