Horizon Collaboration

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.

Results

• 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