Influence of adaptive mesh refinement and the hydro solver on shear-induced mass stripping in a minor-merger scenario
We compare two different codes for simulations of cosmological structure - formation to investigate the sensitivity of hydrodynamical instabilities - to numerics, in particular, the hydro solver and the application of - adaptive mesh refinement (AMR). As a simple test problem, we consider an - init...
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| Main Authors: | , , , , |
|---|---|
| Format: | Article (Journal) |
| Language: | English |
| Published: |
2015
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| In: |
Astronomy and computing
Year: 2014, Volume: 9, Pages: 49-63 |
| ISSN: | 2213-1345 |
| DOI: | 10.1016/j.ascom.2014.11.003 |
| Online Access: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1016/j.ascom.2014.11.003 Verlag, lizenzpflichtig, Volltext: http://adsabs.harvard.edu/abs/2015A%26C.....9...49S |
| Author Notes: | W. Schmidt, J. Schulz, L. Iapichino, F. Vazza, A.S. Almgren |
MARC
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| 245 | 1 | 0 | |a Influence of adaptive mesh refinement and the hydro solver on shear-induced mass stripping in a minor-merger scenario |c W. Schmidt, J. Schulz, L. Iapichino, F. Vazza, A.S. Almgren |
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| 520 | |a We compare two different codes for simulations of cosmological structure - formation to investigate the sensitivity of hydrodynamical instabilities - to numerics, in particular, the hydro solver and the application of - adaptive mesh refinement (AMR). As a simple test problem, we consider an - initially spherical gas cloud in a wind, which is an idealized model for - the merger of a subcluster or galaxy with a big cluster. Based on an - entropy criterion, we calculate the mass stripping from the subcluster - as a function of time. Moreover, the turbulent velocity field is - analyzed with a multi-scale filtering technique. We find remarkable - differences between the commonly used PPM solver with directional - splitting in the ENZO code and an unsplit variant of PPM in the NYX - code, which demonstrates that different codes can converge to - systematically different solutions even when using uniform grids. For - the test case of an unbound cloud, AMR simulations reproduce - uniform-grid results for the mass stripping quite well, although the - flow realizations can differ substantially. If the cloud is bound by a - static gravitational potential, however, we find strong sensitivity to - spurious fluctuations which are induced at the cutoff radius of the - potential and amplified by the bow shock. This gives rise to substantial - deviations between uniform-grid and AMR runs performed with ENZO, while - the mass stripping in NYX simulations of the subcluster is nearly - independent of numerical resolution and AMR. Although many factors - related to numerics are involved, our study indicates that unsplit - solvers with advanced flux limiters help to reduce grid effects and to - keep numerical noise under control, which is important for - hydrodynamical instabilities and turbulent flows. | ||
| 534 | |c 2014 | ||
| 650 | 4 | |a Adaptive mesh refinement | |
| 650 | 4 | |a Hydrodynamics | |
| 650 | 4 | |a Instabilities | |
| 650 | 4 | |a Intracluster medium | |
| 650 | 4 | |a Turbulence | |
| 700 | 1 | |a Schulz, Jochen |d 1976- |e VerfasserIn |0 (DE-588)136659241 |0 (DE-627)585451842 |0 (DE-576)301192928 |4 aut | |
| 700 | 1 | |a Iapichino, Luigi |d 1976- |e VerfasserIn |0 (DE-588)130519634 |0 (DE-627)505285800 |0 (DE-576)298244888 |4 aut | |
| 700 | 1 | |a Vazza, Franco |d 1979- |e VerfasserIn |0 (DE-588)103040206X |0 (DE-627)73522093X |0 (DE-576)37822607X |4 aut | |
| 700 | 1 | |a Almgren, Ann S. |e VerfasserIn |4 aut | |
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