Abstract
In numerical simulations, artificial terms are applied to the evolution equations for stability. To prove their validity, these terms are thoroughly tested in test problems where the results are well known. However, they are seldom tested in production-quality simulations at high resolution where they interact with a plethora of physical and numerical algorithms. We test three artificial resistivities in both the Orszag-Tang vortex and in a star formation simulation. From the Orszag-Tang vortex, the Price et. al. (2017) artificial resistivity is the least dissipative thus captures the density and magnetic features; in the star formation algorithm, each artificial resistivity algorithm interacts differently with the sink particle to produce various results, including gas bubbles, dense discs, and migrating sink particles. The star formation simulations suggest that it is important to rely upon physical resistivity rather than artificial resistivity for convergence.
Original language | English |
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Title of host publication | Proceedings SPHERIC 2017 |
Subtitle of host publication | 12th International SPHERIC Workshop |
Editors | A.J.C. Crespo, M.G. Gesteira, C. Altomare |
Place of Publication | Spain |
Publisher | Universidade de Vigo |
Publication status | Published - 13 Jun 2017 |
Event | 12th International Smoothed Particle Hydrodynamics European Research Interest Community (SPHERIC) Workshop - Ourense, Spain Duration: 13 Jun 2017 → 15 Jun 2017 Conference number: 12 http://spheric2017.uvigo.es/ |
Workshop
Workshop | 12th International Smoothed Particle Hydrodynamics European Research Interest Community (SPHERIC) Workshop |
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Abbreviated title | SPHERIC |
Country/Territory | Spain |
City | Ourense |
Period | 13/06/17 → 15/06/17 |
Internet address |