nIFTy galaxy cluster simulations II: radiative models
Monthly Notices of the Royal Astronomical Society（2016）
摘要
We have simulated the formation of a massive galaxy cluster ($M_{200}^{\rm crit}$ = 1.1 × 1015 h−1 M⊙) in a Λ cold dark matter universe using 10 different codes (ramses, 2 incarnations of arepo and 7 of gadget), modelling hydrodynamics with full radiative subgrid physics. These codes include smoothed-particle hydrodynamics (SPH), spanning traditional and advanced SPH schemes, adaptive mesh and mov...
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关键词
methods: numerical,galaxies: haloes,cosmology: theory,dark matter
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