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DTSTAMP:20210916T132452Z
LOCATION:Lise Girardin
DTSTART;TZID=Europe/Stockholm:20210707T143000
DTEND;TZID=Europe/Stockholm:20210707T150000
UID:submissions.pasc-conference.org_PASC21_sess149_msa324@linklings.com
SUMMARY:Enzo-E: An Exascale AMR Code for Self-Gravitating Astrophysical Fl
 uid Dynamics
DESCRIPTION:Minisymposium\n\nEnzo-E: An Exascale AMR Code for Self-Gravita
 ting Astrophysical Fluid Dynamics\n\nO'Shea, Norman, Bordner\n\nEnzo-E is 
 a new version of the Enzo adaptive mesh refinement fluid dynamics code (ht
 tp://enzo-project.org), which is widely used to study self-gravitating, mu
 ltiphysics astrophysical phenomena such as star and galaxy formation. 
 ; The Enzo-E code is based on the Charm++ parallel programming framework (
 http://charmplusplus.org/), which supports a task-based parallel
  programming paradigm that promotes excellent scaling for simulations of t
 hese types of phenomena.  In this presentation I will discuss the fun
 damental design decisions underlying Enzo-E's development, successes and c
 hallenges to date, and an outlook as the Enzo-E project moves toward the e
 xascale era.  More information about Enzo-E, including the code and d
 ocumentation, can be found at http://cello-project.org/ .\n\nDomain: 
 CS and Math, Physics
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