Hydrodynamical simulations of cosmic structures
Hydrodynamical simulations of cosmic structures
Hydrodynamical simulations of cosmic structures
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GADGET-3 by V. Springel<br />
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Tools<br />
Tree code to solve gravity + PM at large scales<br />
SPH hydro with energy and entropy conserving formulation<br />
refined load balance to work for isolated objects<br />
chemical evolution code<br />
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enrichment <strong>of</strong> several chemical species by SNII, SNIa and AGB<br />
metal cooling <strong>of</strong> gas by interpolating Cloudy tables<br />
AGN feedback<br />
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heating from accreting massive black holes<br />
Energy-driven and momentum-driven winds<br />
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standard and improved implementations<br />
MUlti-Phase Particle Integrator<br />
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star formation and SN feedback<br />
Zoomed-in initial conditions generator<br />
Molecular chemistry and cooling below 10 4 K<br />
Magnetic fields in clusters<br />
WISH LIST: autonomy on initial conditions, radiative transfer...