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Hydrodynamical simulations of cosmic structures

Hydrodynamical simulations of cosmic structures

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Simulating galaxy clusters<br />

cosmological boxes<br />

Role <strong>of</strong> feedback for:<br />

• Physics <strong>of</strong> galaxy<br />

formation<br />

• IGM properties at<br />

low and high-z<br />

• Properties <strong>of</strong> the<br />

ICM<br />

Multi-million CPUh projects granted through DEISA, Gauss and<br />

ISCRA, using SP6 and BlueGene/P (PIs: K. Dolag & S. Borgani)

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