PatchworkWave: A Multipatch Infrastructure for Multiphysics/Multiscale/Multiframe/Multimethod Simulations at Arbitrary Order
arXiv:2002.00088
Abstract
We present an extension of the PatchworkMHD code [1], itself an MHD-capable extension of the Patchwork code [2], for which several algorithms presented here were co-developed. Its purpose is to create a multipatch scheme compatible with numerical simulations of arbitrary equations of motion at any discretization order in space and time. In the Patchwork framework, the global simulation is comprised of an arbitrary number of moving, local meshes, or patches, which are free to employ their own resolution, coordinate system/topology, physics equations, reference frame, and in our new approach, numerical method. Each local patch exchanges boundary data with a single global patch on which all other patches reside through a client-router-server parallelization model. In generalizing Patchwork to be compatible with arbitrary order time integration, PatchworkMHD and PatchworkWave have significantly improved the interpatch interpolation accuracy by removing an interpolation of interpolated data feedback present in the original Patchwork code. Furthermore, we extend Patchwork to be multimethod by allowing multiple state vectors to be updated simultaneously, with each state vector providing its own interpatch interpolation and transformation procedures. As such, our scheme is compatible with nearly any set of hyperbolic partial differential equations. We demonstrate our changes through the implementation of a scalar wave toy-model that is evolved on arbitrary, time dependent patch configurations at 4th order accuracy.
32 pages, 13 figures
References in corpus (13)
- GW170608: Observation of a 19-solar-mass Binary Black Hole Coalescence
- Theory of Core-Collapse Supernovae
- A constrained scheme for Einstein equations based on Dirac gauge and spherical coordinates
- Binary Black-Hole Mergers in Magnetized Disks: Simulations in Full General Relativity
- Binary Black Hole Accretion During Inspiral and Merger
- Covariant formulations of BSSN and the standard gauge
- Characteristic Signatures in the Thermal Emission from Accreting Binary Black Holes
- Binary black hole mergers in gaseous disks: Simulations in general relativity
- Relativistic Dynamics and Mass Exchange in Binary Black Hole Mini-Disks
- Minidisks in Binary Black Hole Accretion
- Quasi-Periodicity of Supermassive Binary Black Hole Accretion Approaching Merger
- DISCO: A 3D Moving-Mesh Magnetohydrodynamics Code Designed for the Study of Astrophysical Disks
- X-ray follow-up of extragalactic transients