Dependence of Inner Accretion Disk Stress on Parameters: The Schwarzschild Case

John Hawley
We explore the parameter dependence of inner disk stress in black hole accretion by contrasting the results of a number of simulations, all employing three-dimensional general relativistic MHD in a Schwarzschild spacetime. Five of these simulations were performed with the intrinsically conservative code HARM3D, which allows careful regulation of the disk aspect ratio, H/R; our simulations span a range in H/R from 0.06 to 0.17. We contrast these simulations with two previously reported simulations in...
This data repository is not currently reporting usage information. For information on how your repository can submit usage information, please see our documentation.