ENZO: An Adaptive Mesh Refinement Code for Astrophysics (Version 2.6)
Corey Brummel-SmithCenter for Relativistic Astrophysics , School of Physics , Georgia Institute of TechnologyGreg L. BryanDept. of Astronomy , Columbia UniversityIryna S. ButskyDept. of Astronomy , University of Washington in SeattleLauren CorliesDept. of Physics and Astronomy, Johns Hopkins UniversityAndrew EmerickAmerican Museum of Natural HistoryJohn C. ForbesCenter for Astrophysics , Harvard & SmithsonianYusuke FujimotoUniversity of Hamburg RSAA ,Nathan GoldbaumSchool of Information Sciences , University of Illinois , Urbana-ChampaignPhilipp GreteDept. of Physics and Astronomy , Michigan State UniversityCameron HummelsCalifornia Institute of TechnologyJi-hoon KimSeoul National University , KoreaDaegene KohKavli Institute for Particle Astrophysics and Cosmology , Stanford UniversityMiao LiCenter for Computational Astrophysics , Flatiron InstituteYuan LiTheoretical Astrophysics Center, University of California BerkeleyXinyu LiColumbia UniversityBrian W. O’SheaDept. of Physics and Astronomy , Michigan State UniversityMolly S. PeeplesDept. of Physics and Astronomy, Johns Hopkins UniversityJohn A. ReganCenter for Astrophysics and Relativity , Dublin City UniversityM. SalemDept. of Astronomy , Columbia UniversityW. SchmidtHamburg Observatory, University of HamburgChristine M. SimpsonEnrico Fermi Institute, The University of ChicagoBritton SmithRoyal Observatory , University of EdinburghJason TumlinsonSpace Telescope Science InstituteMatthew TurkSchool of Information Sciences , University of Illinois , Urbana-ChampaignJohn WiseInternational Center for Relativistic Astrophysics NetworkTom AbelDepartment of Physics , Stanford University , StanfordJames BordnerCenter for Astrophysics and Space Sciences, University of California, San DiegoRenyue CenDepartment of Astrophysical Sciences , Princeton UniversityDavid C. CollinsDept. of Physics , Florida State UniversityBrian D. CrosbyDept. of Physics and Astronomy, Michigan State UniversityP. V. F. EdelmannMax-Planck-Institut for Astrophysik 33 Hamburg Observatory ,Oliver HahnObservatoire de la C'ote d'AzurRobert P. HarknessCenter for Astrophysics and Space Sciences, University of California, San DiegoElizabeth Harper-ClarkCanadian Institute for Theoretical AstrophysicsShuo KongObservatoire de la C'ote d'AzurAlexei G. KritsukCenter for Astrophysics and Space Sciences , University of California , San DiegoM. KuhlenTheoretical Astrophysics Center , University of California Berkeley 30 OnSpot Data 31James LarrueObservatoire de la C'ote d'AzurEve J. LeeObservatoire de la C'ote d'AzurGreg MeeceDept. of Physics and Astronomy, Michigan State UniversityMichael L. NormanCenter for Astrophysics and Space Sciences, University of California, San DiegoJeffrey S. OishiPhysics and Astronomy, Bates College 14 Dept. of Astronomy, University of Washington in SeattleP. PaschosCenter for Astrophysics and Space Sciences, University of California, San DiegoCarolyn PerutaDept. of Physics and Astronomy , Michigan State UniversityAlex RazoumovDept. of Astronomy & Physics, Saint Mary's University, HalifaxDaniel R. ReynoldsDepartment of Mathematics , Southern Methodist UniversityDevin W. SilviaDepartment of Computational Mathematics, Science, and Engineering , Michigan State UniversitySamuel W. SkillmanDescartes LabsStephen SkoryObservatoire de la C'ote d'AzurGeoffrey C. SoCenter for Astrophysics and Space Sciences , University of California , San DiegoElizabeth J. TaskerInstitute of Space and Astronautical Science , Japan Aerospace Exploration AgencyRick WagnerCenter for Astrophysics and Space Sciences, University of California, San DiegoPeng WangKavli Institute for Particle Astrophysics and Cosmology , Stanford UniversityHao XuCenter for Astrophysics and Space Sciences, University of California, San DiegoFen ZhaoSaint Mary's University , Halifax
2019en
ABI
Annotatsiya
Enzo (Enzo Developers, 2019a) is a block-structured adaptive mesh refinement code that is widely used to simulate astrophysical fluid flows (primarily, but not exclusively, cosmological structure formation, star formation, and turbulence).The code is a community project with dozens of users, and has contributed to hundreds of peer-reviewed publications in astrophysics, physics, and computer science.The code utilizes a Cartesian mesh can be run in one, two, or
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