Abstract: Enzo is an adaptive mesh refinement (AMR), grid-based hybrid code (hydro + N-Body) which is designed to do simulations of cosmological structure formation. It uses the algorithms of Berger & Collela to improve spatial and temporal resolution in regions of large gradients, such as gravitationally collapsing objects. The Enzo simulation software is incredibly flexible, and can be used to simulate a wide range of cosmological situations with the available physics packages.
Enzo has been parallelized using the MPI message-passing library and can run on any shared or distributed memory parallel supercomputer or PC cluster. Simulations using as many as 1024 processors have been successfully carried out on the San Diego Supercomputing Center's Blue Horizon, an IBM SP.
Credit: O'Shea, Brian W.; Bryan, Greg; Bordner, James; Norman, Michael L.; Abel, Tom; Harkness, Robert; Kritsuk, Alexei
Preferred citation method: https://ui.adsabs.harvard.edu/abs/2014ApJS..211...19B, a footnote to http://enzo-project.org, and text in CITATION file <a href="https://github.com/enzo-project/enzo-de ... N">here</a>.