The effect of local universe constraints on halo abundance and clustering
Cosmological N-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 is, however, possi...
| Päätekijät: | , , , |
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| Aineistotyyppi: | Internet publication |
| Kieli: | English |
| Julkaistu: |
Cornell University
2022
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