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20 April 2024
 
  » arxiv » 1307.2265

 Article overview


Enzo: An Adaptive Mesh Refinement Code for Astrophysics
Enzo Collaboration ; Greg L. Bryan ; Michael L. Norman ; Brian W. O'Shea ; Tom Abel ; John H. Wise ; Matthew J. Turk ; Daniel R. Reynolds ; David C. Collins ; Peng Wang ; Samuel W. Skillman ; Britton Smith ; Robert P. Harkness ; James Bordner ; Ji-hoon Kim ; Michael Kuhlen ; Hao Xu ; Nathan Goldbaum ; Cameron Hummels ; Alexei G. Kritsuk ; Elizabeth Tasker ; Stephen Skory ; Christine M. Simpson ; Oliver Hahn ; Jeffrey S. Oishi ; Geoffrey C So ; Fen Zhao ; Renyue Cen ; Yuan Li ;
Date Mon, 8 Jul 2013 20:42:32 GMT (1826kb)
AbstractThis 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.
Source arXiv, 1307.2265
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