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Reducing noise in moving-grid codes with strongly-centroidal Lloyd mesh regularization

, , , , , and . (2015)cite arxiv:1503.07868Comment: 9 pages, 14 figures, MNRAS submitted.

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Correspondence between constrained transport and vector potential methods for magnetohydrodynamics.. J. Comput. Phys., (2017)Galaxy Formation with BECDM -- II. Cosmic Filaments and First Galaxies, , , , , , , , , and 4 other author(s). (2019)cite arxiv:1911.05746Comment: 19 pages, 12 figures, submitted to MNRAS.A Constrained Transport Scheme for MHD on Unstructured Static and Moving Meshes, , and . (2014)cite arxiv:1402.5963Comment: 13 pages, 9 figures, submitted to MNRAS. Animations available at http://www.cfa.harvard.edu/~pmocz/research.html.Smoothed Particle Hydrodynamics: Theory, Implementation, and Application to Toy Stars. Applied Math 205 Final Project, Harvard University, Fall 2011, Prof. Knezevic, (2011)Reducing noise in moving-grid codes with strongly-centroidal Lloyd mesh regularization, , , , , and . (2015)cite arxiv:1503.07868Comment: 9 pages, 14 figures, MNRAS submitted.The large-scale properties of simulated cosmic magnetic fields, , , and . (May 29, 2015)Dynamical Friction in a Fuzzy Dark Matter Universe, , , , , and . (2019)cite arxiv:1909.06381Comment: 41 pages, 11 figures.First star-forming structures in fuzzy cosmic filaments, , , , , , , , , and 3 other author(s). (2019)cite arxiv:1910.01653Comment: 6 pages, 2 figures, accepted to Phys. Rev. Lett.