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.
- Global Radiation Magneto-hydrodynamic Simulations of Sub-Eddington Accretion Disks around Supermassive Black Holes July 9, 2019
- A fourth-order accurate finite volume method for ideal MHD via upwind constrained transport July 9, 2019
- Shearing-box simulations of MRI-driven turbulence in weakly collisional accretion discs July 9, 2019