Enzo: An Adaptive Mesh Refinement Code for Astrophysics
Enzo: An Adaptive Mesh Refinement Code for Astrophysics
This paper describes the open-source code Enzo, which uses block-structured adaptive mesh refinement to provide high spatial and temporal resolution for modeling astrophysical fluid flows. The code is Cartesian, can be run in 1, 2, and 3 dimensions, and supports a wide variety of physics including hydrodynamics, ideal and non-ideal magnetohydrodynamics, N-body dynamics (and, more broadly, self-gravity of fluids and particles), primordial gas chemistry, optically-thin radiative cooling of primordial and metal-enriched plasmas (as well as some optically-thick cooling models), radiation transport, cosmological expansion, and models for star formation and feedback in a cosmological context. In addition to explaining the algorithms implemented, we present solutions for a wide range of test problems, demonstrate the code's parallel performance, and discuss the Enzo collaboration's code development methodology.
Geoffrey C So、Hao Xu、Greg L. Bryan、Fen Zhao、Brian W. O'Shea、Ji-hoon Kim、Matthew J. Turk、Cameron Hummels、The Enzo Collaboration、Peng Wang、Yuan Li、Elizabeth Tasker、James Bordner、David C. Collins、Oliver Hahn、Daniel R. Reynolds、John H. Wise、Britton Smith、Stephen Skory、Jeffrey S. Oishi、Alexei G. Kritsuk、Christine M. Simpson、Nathan Goldbaum、Michael Kuhlen、Renyue Cen、Robert P. Harkness、Michael L. Norman、Tom Abel、Samuel W. Skillman
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Geoffrey C So,Hao Xu,Greg L. Bryan,Fen Zhao,Brian W. O'Shea,Ji-hoon Kim,Matthew J. Turk,Cameron Hummels,The Enzo Collaboration,Peng Wang,Yuan Li,Elizabeth Tasker,James Bordner,David C. Collins,Oliver Hahn,Daniel R. Reynolds,John H. Wise,Britton Smith,Stephen Skory,Jeffrey S. Oishi,Alexei G. Kritsuk,Christine M. Simpson,Nathan Goldbaum,Michael Kuhlen,Renyue Cen,Robert P. Harkness,Michael L. Norman,Tom Abel,Samuel W. Skillman.Enzo: An Adaptive Mesh Refinement Code for Astrophysics[EB/OL].(2013-07-08)[2025-07-01].https://arxiv.org/abs/1307.2265.点此复制
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