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Fluids in the Universe: Adaptive Mesh Refinement in Cosmology
March/April 1999 (vol. 1 no. 2)
pp. 46-53
| ASCII Text | x | ||
| Greg L. Bryan, "Fluids in the Universe: Adaptive Mesh Refinement in Cosmology," Computing in Science and Engineering, vol. 1, no. 2, pp. 46-53, March/April, 1999. | |||
| BibTex | x | ||
| @article{ 10.1109/5992.753046, author = {Greg L. Bryan}, title = {Fluids in the Universe: Adaptive Mesh Refinement in Cosmology}, journal ={Computing in Science and Engineering}, volume = {1}, number = {2}, issn = {1521-9615}, year = {1999}, pages = {46-53}, doi = {http://doi.ieeecomputersociety.org/10.1109/5992.753046}, publisher = {IEEE Computer Society}, address = {Los Alamitos, CA, USA}, } | |||
| RefWorks Procite/RefMan/Endnote | x | ||
| TY - MGZN JO - Computing in Science and Engineering TI - Fluids in the Universe: Adaptive Mesh Refinement in Cosmology IS - 2 SN - 1521-9615 SP46 EP53 EPD - 46-53 A1 - Greg L. Bryan, PY - 1999 VL - 1 JA - Computing in Science and Engineering ER - | |||
DOI Bookmark: http://doi.ieeecomputersociety.org/10.1109/5992.753046
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.
Citation:
Greg L. Bryan, "Fluids in the Universe: Adaptive Mesh Refinement in Cosmology," Computing in Science and Engineering, vol. 1, no. 2, pp. 46-53, March-April 1999, doi:10.1109/5992.753046
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