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Over the past two decades, high-performance computing has revolutionized astrophysics. On the theory side, simulations running in parallel on hundreds or thousands of processors have made it possible to understand the formation of large-scale structure in the Universe, the growth of supermassive black holes in the centers of galaxies, the formation of earth-like planets around Sun-like stars, and the nature of the first stars and galaxies.

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Institute for Theory and Computation
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