Physics problems are in general very difficult to solve exactly. This is due to several reasons: lack of algebraic or analytic solubility, complexity, and chaos.

UV HPC deploying SGI high performance computing solutions allow astrophysicists, high energy physicists, plasma physicists, geophysicists and other physical scientists to more rapidly simulate complex phenomena and analyze large amounts of experimental data.

Theoreticians require advanced computation and huge volumes of storage and compute intensive systems to increase understanding of the behavior of systems ranging from the sub-atomic to stars, galaxies and beyond, while experimentalists increasingly rely on advanced storage systems to accommodate and make sense of the mountains of data ingested from an ever growing array of specialized instrumentation.

Common workloads involve:

• AMUSE

• ART

• Chemora

• Chroma

• ENZO

• FLASH

• GADGET

• GTC

• GTS

• MILC

• MODEST

• RAMSES

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