Simulating gravitational motion, gas dynamics, and structure in the cosmos
arXiv:2302.01895 · doi:10.1119/5.0144906
Abstract
We provide introductory explanations and illustrations of the -body hydrodynamics code Charm N-body GrAvity solver (ChaNGa). ChaNGa simulates the gravitational motion and gas dynamics of matter in space, with the goal of modeling galactic and/or cosmological structure and evolution. We discuss the algorithm for leapfrog integration and smoothed particle hydrodynamics and computer science concepts used by the program, including the binary data structure for the particle positions. Our presentation borrows from the doctoral dissertation of J.\ G.\ Stadel. Problems are provided in order to use ChaNGa to learn or solidify some cosmological concepts.
arXiv commentAccepted by the American Journal of Physics. Two important supplementary documents are included
References in corpus (13)
- Planck 2015 results. XIII. Cosmological parameters
- The cosmological simulation code GADGET-2
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
- Galaxies on FIRE (Feedback In Realistic Environments): Stellar Feedback Explains Cosmologically Inefficient Star Formation
- First results from the IllustrisTNG simulations: A tale of two elements -- chemical evolution of magnesium and europium
- Multi-scale initial conditions for cosmological simulations
- Gasoline: An adaptable implementation of TreeSPH
- Dark matter and cosmic structure
- Gasoline2: A Modern SPH Code
- The AGORA High-Resolution Galaxy Simulations Comparison Project. II: Isolated Disk Test
- Cold Filamentary Accretion and the Formation of Metal Poor Globular Clusters and Halo Stars
- An optimum time-stepping scheme for N-body simulations
- How to bend galaxy disc profiles II: stars surfing the bar in Type-III discs