Lecture Notes in Computer Science
DOI: 10.1007/978-3-540-71351-7_37
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Scalable Cosmological Simulations on Parallel Machines

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Cited by 11 publications
(12 citation statements)
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“…The first one is wave2D, which uses a finite differencing scheme to calculate pressure information over a discretized 2D grid. The second application, ChaNGa, is for N-Body based parallel simulations and is used in cosmology and astronomy [12].…”
Section: Experiments and Analysismentioning
confidence: 99%
“…The first one is wave2D, which uses a finite differencing scheme to calculate pressure information over a discretized 2D grid. The second application, ChaNGa, is for N-Body based parallel simulations and is used in cosmology and astronomy [12].…”
Section: Experiments and Analysismentioning
confidence: 99%
“…For each application, less than 0.5% of the application code was affected. ChaNGa [19], [20] is a code for performing collisionless N-body simulations. It simulates cosmological phenomena with periodic boundary conditions in comoving coordinates or isolated stellar systems.…”
Section: Application Resultsmentioning
confidence: 99%
“…Processor virtualization also enables runtime measurement based dynamic load balancing. The idea has been useful in numerous applications from molecular dynamics [21] to cosmology [14]. AMPI is an implementation of MPI on top of the Charm++ runtime system that allows traditional MPI codes to reap the benefits of virtualization such as latency tolerance and runtime load balancing.…”
Section: Related Workmentioning
confidence: 99%