Accurately simulating anisotropic thermal conduction on a moving mesh
arXiv:1512.03053 · doi:10.1093/mnras/stw294
Abstract
We present a novel implementation of an extremum preserving anisotropic diffusion solver for thermal conduction on the unstructured moving Voronoi mesh of the AREPO code. The method relies on splitting the one-sided facet fluxes into normal and oblique components, with the oblique fluxes being limited such that the total flux is both locally conservative and extremum preserving. The approach makes use of harmonic averaging points and a simple, robust interpolation scheme that works well for strong heterogeneous and anisotropic diffusion problems. Moreover, the required discretisation stencil is small. Efficient fully implicit and semi-implicit time integration schemes are also implemented. We perform several numerical tests that evaluate the stability and accuracy of the scheme, including applications such as point explosions with heat conduction and calculations of convective instabilities in conducting plasmas. The new implementation is suitable for studying important astrophysical phenomena, such as the conductive heat transport in galaxy clusters, the evolution of supernova remnants, or the distribution of heat from blackhole-driven jets into the intracluster medium.
17 pages, 16 figures, Submitted to MNRAS
References in corpus (12)
- SPLASH: An interactive visualisation tool for Smoothed Particle Hydrodynamics simulations
- Regulation of star formation in giant galaxies by precipitation, feedback, and conduction
- A scheme for radiation pressure and photon diffusion with the M1 closure in RAMSES-RT
- Cosmic ray feedback in hydrodynamical simulations of galaxy formation
- Preserving Monotonicity in Anisotropic Diffusion
- Buoyancy Instabilities in Weakly Magnetized Low Collisionality Plasmas
- Cooling Time, Freefall Time, and Precipitation in the Cores of ACCEPT Galaxy Clusters
- An implementation of radiative transfer in the cosmological simulation code GADGET
- Conduction and the Star-Formation Threshold in Brightest Cluster Galaxies
- Nonlinear Simulations of the Heat Flux Driven Buoyancy Instability and its Implications for Galaxy Clusters
- Simulating Anisotropic Thermal Conduction in Supernova Remnants, Implications for the Interstellar Medium
- Numerical simulations of buoyancy instabilities in galaxy cluster plasmas with cosmic rays and anisotropic thermal conduction
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