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.
- Magnetorotational Turbulence and Dynamo in a Collisionless Plasma September 3, 2017
- Extended general relativistic magnetohydrodynamics: Formulation and application to black hole accretion September 3, 2017
- Development and application of numerical techniques for general-relativistic magnetohydrodynamics simulations of black hole accretion September 3, 2017