Abstract
We present a new general relativistic magnetohydrodynamics (GRMHD) code integrated into the Athena++ framework. Improving upon the techniques used in most GRMHD codes, ours allows the use of advanced, less diffusive Riemann solvers, in particular HLLC and HLLD. We also employ a staggered-mesh constrained transport algorithm suited for curvilinear coordinate systems in order to maintain the divergence-free constraint of the magnetic field. Our code is designed to work with arbitrary stationary spacetimes in one, two, or three dimensions, and we demonstrate its reliability through a number of tests. We also report on its promising performance and scalability.
| Original language | English (US) |
|---|---|
| Article number | 22 |
| Journal | Astrophysical Journal, Supplement Series |
| Volume | 225 |
| Issue number | 2 |
| DOIs | |
| State | Published - Aug 2016 |
Keywords
- accretion, accretion disks
- black hole physics
- magnetohydrodynamics (MHD)
- relativistic processes
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
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