GenASiS: General Astrophysical Simulation System. I. Refinable Mesh and Nonrelativistic Hydrodynamics
arXiv:1207.3392 · doi:10.1088/0067-0049/210/2/17
Abstract
GenASiS (General Astrophysical Simulation System) is a new code being developed initially and primarily, though by no means exclusively, for the simulation of core-collapse supernovae on the world's leading capability supercomputers. This paper---the first in a series---demonstrates a centrally refined coordinate patch suitable for gravitational collapse and documents methods for compressible nonrelativistic hydrodynamics. We benchmark the hydrodynamics capabilities of GenASiS against many standard test problems; the results illustrate the basic competence of our implementation, demonstrate the strengths and limitations of the HLLC relative to the HLL Riemann solver in a number of interesting cases, and provide preliminary indications of the code's ability to scale and to function with cell-by-cell fixed-mesh refinement.
Belated update to version accepted ApJS
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Cited by in corpus (8)
- Stochasticity and efficiency of simplified core-collapse supernova explosions
- A simple, entropy-based dissipation trigger for SPH
- Targeting GPUs with OpenMP Directives on Summit: A Simple and Effective Fortran Experience
- APSARA: A multi-dimensional unsplit fourth-order explicit Eulerian hydrodynamics code for arbitrary curvilinear grids
- thornado-hydro: a discontinuous Galerkin method for supernova hydrodynamics with nuclear equations of state
- GenASiS Basics: Object-oriented utilitarian functionality for large-scale physics simulations (Version 4)
- GenASiS Mathematics: Object-oriented manifolds, operations, and solvers for large-scale physics simulations
- GenASiS: General Astrophysical Simulation System. II. Self-gravitating Baryonic Matter