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Smoothed Particle Radiation Hydrodynamics: Two-Moment method with Local Eddington Tensor Closure

, , , and . (2021)cite arxiv:2102.08404Comment: 31 pages, 20 figures; submitted to MNRAS; Comments welcome.

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The Impact of Baryonic Physics on the Structure of Dark Matter Halos: the View from the FIRE Cosmological Simulations, , , , , , and . (2015)cite arxiv:1507.02282Comment: 23 pages, 14 figures, submitted to MNRAS.FIRE-2 Simulations: Physics versus Numerics in Galaxy Formation, , , , , , , , , and 18 other author(s). (2017)cite arxiv:1702.06148Comment: 66 pages, 39 figures. Simulation animations and visualizations available at http://www.tapir.caltech.edu/~phopkins/Site/animations and http://fire.northwestern.edu Paper includes complete FIRE algorithms and public ICs (http://www.tapir.caltech.edu/~phopkins/publicICs).Smoothed Particle Radiation Hydrodynamics: Two-Moment method with Local Eddington Tensor Closure, , , and . (2021)cite arxiv:2102.08404Comment: 31 pages, 20 figures; submitted to MNRAS; Comments welcome.An FPGA Implementation of GENET for Solving Graph Coloring Problems ., , , , , , , and . FCCM, page 284-285. IEEE Computer Society, (1998)Metal flows of the circumgalactic medium, and the metal budget in galactic halos, , , , , , , , , and 1 other author(s). (2016)cite arxiv:1606.09252Comment: 18 Pages, 14 Figures, Submitted to MNRAS, comments welcome.On the deuterium abundance and the importance of stellar mass loss in the interstellar and intergalactic medium, , , , , , , and . (2017)cite arxiv:1704.08254Comment: Submitted to MNRAS. Comments welcome.What FIREs Up Star Formation: the Emergence of the Kennicutt-Schmidt Law from Feedback, , , , , , , , and . (2017)cite arxiv:1701.01788Comment: 15 pages, 10 figures, submitted to MNRAS.Low-Redshift Lyman Limit Systems as Diagnostics of Cosmological Inflows and Outflows, , , , , , , , and . (2016)cite arxiv:1608.05712Comment: 13 pages, 12 figures. Submitted.When the Jeans don't fit: How stellar feedback drives stellar kinematics and complicates dynamical modeling in low-mass galaxies, , , , , , , and . (2016)cite arxiv:1610.04232Comment: Submitted to ApJ. Main results in Figures 3, 7, and 8.Remote monitoring on capacity of portable power bank in testing laboratories., , , and . IECON, page 4734-4739. IEEE, (2017)