Abstract: HARMPI is a parallel, 3D version of HARM (ascl:1209.005), which solves hyperbolic partial differential equations in conservative form using high-resolution shock-capturing techniques. The code is parallelized using MPI and is fully operational in 3D. HARMPI, like HARM, is capable of using non-uniform grids and solves the relativistic magnetohydrodynamic equations of motion on a stationary black hole spacetime in Kerr-Schild coordinates to evolve an accretion disk model.
Credit: Tchekhovskoy, Alexander
Preferred citation method: https://ui.adsabs.harvard.edu/abs/2003ApJ...589..444G and https://ui.adsabs.harvard.edu/abs/2006ApJ...641..626N