The effect of local Universe constraints on halo abundance and clustering

The effect of local Universe constraints on halo abundance and clustering

Čájet eará veršuvnnaid (1)

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...

Bibliográfalaš dieđut
Váldodahkkit:	Hutt, ML, Desmond, H, Devriendt, J, Slyz, A
Materiálatiipa:	Journal article
Giella:	English
Almmustuhtton:	Oxford University Press 2022

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