Hydrodynamic Simulations
Hydrodynamic Simulations is a computational methodology in numerical astrophysics that models the time evolution of fluid dynamics in astrophysical systems by numerically solving the hydrodynamic equations, particularly applied to phenomena such as supernova remnants to capture shocks, turbulence, and mass transfer in gaseous media.
3.9K
Publications
294.5K
Citations
8.6K
Authors
1.8K
Institutions
Publications per year
2017–2026
1.1K
Variants
Hydrodynamic Simulation
3.9K
Smoothed Particle Hydrodynamics
J. J. Monaghan · Annual Review of Astronomy and Astrophysics · 1992 · 4.9K citations
Smoothed particle hydrodynamics
J. J. Monaghan · Reports on Progress in Physics · 2005 · 2.7K citations
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8.6K
Center for Astrophysics Harvard & Smithsonian, United States
64 publications · 10.9K citations
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26
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1.8K
Max Planck Institute for Astrophysics
Garching, Germany
86 h-index
383 publications
61.1K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
69 h-index
306 publications
38.8K citations
University of California, Berkeley
Berkeley, United States
63 h-index
175 publications
25.4K citations

Centre National de la Recherche Scientifique
Paris, France
62 h-index
667 publications
29.9K citations
Princeton University
Princeton, United States
59 h-index
247 publications
25.8K citations

Lawrence Livermore National Laboratory
Livermore, United States
55 h-index
823 publications
54.6K citations
University of Arizona
Tucson, United States
55 h-index
177 publications
18.3K citations
Los Alamos National Laboratory
Los Alamos, United States
51 h-index
459 publications
24.6K citations
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ApJ · 736 publications · 58.4K citations
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724 publications · 69.5K citations
121
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181 publications · 13.8K citations
62
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PRL · 85 publications · 7.5K citations
46
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60 publications · 12K citations
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