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Hydrodynamical simulations of cosmic structures

Hydrodynamical simulations of cosmic structures

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Simulating the IGM<br />

IGM astrophysics:<br />

Statistics <strong>of</strong> Lyman-alpha<br />

forest<br />

Thermal and chemical<br />

properties <strong>of</strong> the IGM<br />

Role <strong>of</strong> galaxy outflows and<br />

their detectability as metal<br />

absorbers<br />

-> IGM (D'Odorico's talk)<br />

-> Cosmology with Lymanalpha<br />

forest (Viel's talk)<br />

Do we understand inflows<br />

and outflows <strong>of</strong> baryons?

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