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Computing highlights
Studying supernova shock waves
Dr John Blondin
The compute speed of the VH-1 hydrodynamics code used to study the dynamics of the stalled supernova shock wave in three dimensions in the TSI project.
This plot shown in the graph left represents a "weak" scaling study, in which the computational workload (i.e. the size of the problem) is increased along with the number of processors. The test problem that was used involves a strong shock wave propagating across the volume of a cartesian box.
A typical TSI run uses of the order of one billion zones, and a full time update can be performed in roughly 1s on either of the new Cray platforms.
Dr John Blondin is Professor of Physics at North Carolina State University.