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Phantom: A smoothed particle hydrodynamics and magnetohydrodynamics code for astrophysics

, , , , , , , , , , , , , , , , , , , , , , , , , and . (2017)cite arxiv:1702.03930Comment: 77 pages, 51 figures, 335 equations, submitted to PASA. Code available from https://phantomsph.bitbucket.io/.

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Phantom: A smoothed particle hydrodynamics and magnetohydrodynamics code for astrophysics, , , , , , , , , and 16 other author(s). (2017)cite arxiv:1702.03930Comment: 77 pages, 51 figures, 335 equations, submitted to PASA. Code available from https://phantomsph.bitbucket.io/.Self-induced dust traps: overcoming planet formation barriers, , and . Monthly Notices of the Royal Astronomical Society, (Jan 4, 2017)ALMA images of discs: are all gaps carved by planets?, , , , and . (Sep 2, 2015)Dynamics of dust grains in turbulent molecular clouds. Conditions for decoupling and limits of different numerical implementations, , , , , and . (2023)cite arxiv:2301.04946Comment: 22 pages, 16 figures, accepted for publication in A&A.Fast and accurate Voronoi density gridding from Lagrangian hydrodynamics data., , and . J. Comput. Phys., (2018)Two mechanisms for dust gap opening in protoplanetary discs, , , and . (Feb 24, 2016)Is the dust-to-gas ratio constant in molecular clouds?, , and . Monthly Notices of the Royal Astronomical Society: Letters, (Jun 15, 2017)Grand challenges in protoplanetary disc modelling, , , , , , , , , and 11 other author(s). Publications of the Astronomical Society of Australia, (Sep 20, 2016)