dark matter haloes 暗物质晕
Then, we analyse in detail the mass-accretion histories and structural properties of dark haloes in high-resolution N-body simulations.
本文利用高分辨率的N体数值模拟仔细分析了暗晕的质量吸积历史和内部结构演化历史。
Compared with the PL-CDM model, the RSI-CDM model can raise the mass abundance of dark haloes for small mass haloes at lower redshifts, but it is not apparent on scales of massive mass haloes.
与PL - CDM相比，RSI - CDM在低红移处小质量暗晕的质量丰度较大，但在大结构质量晕中两者差别不明显，而且这个差异随着红移降低而增大。
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