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.
- grim: A Flexible, Conservative Scheme for Relativistic Fluid Theories September 10, 2016
- Large-Eddy Simulations of Magnetohydrodynamic Turbulence in Heliophysics and Astrophysics September 10, 2016
- Iron Opacity Bump Changes the Stability and Structure of Accretion Disks in Active Galactic Nuclei September 10, 2016