About the Group
The horizon collaboration’s goal is to develop computational tools for generating state of the art, relativistic, ab initio models of accreting black holes – from the interstellar medium to the event horizon.
- GRMHD in Athena++ Using Advanced Riemann Solvers and Staggered-Mesh Constrained Transport November 16, 2015
- Evolution of Accretion Discs around a Kerr Black Hole using Extended Magnetohydrodynamics November 16, 2015
- Polarized Synchrotron Emissivities and Absorptivities for Relativistic Thermal, Power-Law, and Kappa Distribution Functions November 12, 2015