Abstract: EBHLIGHT solves the equations of general relativistic radiation magnetohydrodynamics in stationary spacetimes. Fluid integration is performed with the second order shock-capturing scheme HARM (ascl:1209.005) and frequency-dependent radiation transport is performed with the second order Monte Carlo code grmonty (ascl:1306.002). Fluid and radiation exchange four-momentum in an explicit first-order operator-split fashion.
Credit: Ryan, Benjamin R.; Dolence, Joshua C.; Gammie, Charles F.; Ressler, Sean M.; Miller, Jonah
Preferred citation method: https://ui.adsabs.harvard.edu/abs/2015ApJ...807...31R