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Testing hydrodynamics schemes in galaxy disc simulations

Few, C. G.; Dobbs, C.; Pettitt, A.; Konstandin, L.

Authors

C. Dobbs

A. Pettitt

L. Konstandin



Abstract

We examine how three fundamentally different numerical hydrodynamics codes follow the evolution of an isothermal galactic disc with an external spiral potential. We compare an adaptive mesh refinement code (RAMSES), a smoothed particle hydrodynamics code (SPHNG), and a volume-discretised meshless code (GIZMO). Using standard refinement criteria, we find that RAMSES produces a disc that is less vertically concentrated and does not reach such high densities as the SPHNG or gizmo runs. The gas surface density in the spiral arms increases at a lower rate for the RAMSES simulations compared to the other codes. There is also a greater degree of substructure in the SPHNG and GIZMOruns and secondary spiral arms are more pronounced. By resolving the Jeans’ length with a greater number of grid cells we achieve more similar results to the Lagrangian codes used in this study. Other alterations to the refinement scheme (adding extra levels of refinement and refining based on local density gradients) are less successful in reducing the disparity between RAMSES and SPHNG/GIZMO. Although more similar, SPHNG displays different density distributions and vertical mass profiles to all modes of gizmo (including the smoothed particle hydrodynamics version). This suggests differences also arise which are not intrinsic to the particular method but rather due to its implementation. The discrepancies between codes (in particular, the densities reached in the spiral arms) could potentially result in differences in the locations and timescales for gravitational collapse, and therefore impact star formation activity in more complex galaxy disc simulations.

Citation

Few, C. G., Dobbs, C., Pettitt, A., & Konstandin, L. (2016). Testing hydrodynamics schemes in galaxy disc simulations. Monthly notices of the Royal Astronomical Society, 460(4), 4382-4396. https://doi.org/10.1093/mnras/stw1226

Journal Article Type Article
Acceptance Date May 19, 2016
Online Publication Date May 26, 2016
Publication Date Aug 21, 2016
Deposit Date Jun 8, 2016
Publicly Available Date Jun 8, 2016
Journal Monthly notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 460
Issue 4
Pages 4382-4396
DOI https://doi.org/10.1093/mnras/stw1226
Keywords Methods: numerical, Hydrodynamics, Galaxies: evolution, Galaxies: structure
Public URL https://hull-repository.worktribe.com/output/439232
Publisher URL mnras.oxfordjournals.org/cgi/reprint/stw1226?ijkey=sYRlx0nJzMU8prB&keytype=ref
Additional Information Copy of article first published in: Monthly notices of the Royal Astronomical Society, 2016, v.460 issue 4.

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Copyright Statement
© 2016 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.





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