DocumentCode :
1488129
Title :
Fluids in the universe: adaptive mesh refinement in cosmology
Author :
Bryan, Greg L.
Author_Institution :
MIT, Cambridge, MA, USA
Volume :
1
Issue :
2
fYear :
1999
Firstpage :
46
Lastpage :
53
Abstract :
Using galactic clusters, galactic formation, and the first stars as examples, the author demonstrates how adaptive mesh refinement techniques can be successfully applied to cosmological research. The method combines adaptive refinement of interesting regions with modern grid-based methods for solving hydrodynamic equations
Keywords :
astronomy computing; clusters of galaxies; cosmology; hydrodynamics; mesh generation; adaptive mesh refinement; cosmic evolution; cosmology; first stars; galactic clusters; galactic formation; grid-based methods; hydrodynamic equations; Adaptive mesh refinement; Computational fluid dynamics; Computational modeling; Equations; Fluctuations; Gravity; Hydrodynamics; Lagrangian functions; Predictive models; Timing;
fLanguage :
English
Journal_Title :
Computing in Science & Engineering
Publisher :
ieee
ISSN :
1521-9615
Type :
jour
DOI :
10.1109/5992.753046
Filename :
753046
Link To Document :
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