Hydrodynamical simulations of cosmic structures
Hydrodynamical simulations of cosmic structures
Hydrodynamical simulations of cosmic structures
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Zoom-in <strong>simulations</strong> <strong>of</strong> 45 individual halos (5e10-2e13M⊙)<br />
Hirschmann et al. in preparation<br />
Can we produce<br />
realistic galaxy<br />
populations?<br />
Ongoing project: simulation <strong>of</strong> 36 Mpc/h box with 512 3 gas + 512 3 DM particles and<br />
128 outputs, with several star formation & SN feedback models, granted by<br />
CASPUR and proposed to CINECA (PI: Murante & Monaco)<br />
-> chemical evolution (De Lucia's talk)<br />
-> SED synthesis (De Lucia's talk)<br />
-> observations <strong>of</strong> galaxies (Tozzi's talk)
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