The effect of local Universe constraints on halo abundance and clustering
Cosmological <i>N</i>-body simulations of the dark matter component of the universe typically use initial conditions with a fixed power spectrum and random phases of the density field, leading to structure consistent with the local distribution of galaxies only in a statistical sense. It...
| المؤلفون الرئيسيون: | , , , |
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| التنسيق: | Journal article |
| اللغة: | English |
| منشور في: |
Oxford University Press
2022
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