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- W2065201732 abstract "Much evidence suggests that we live in a flat cold dark matter universe with a cosmological constant. Accurate analytic formulae are now available for many properties of the dark halo population in such a Universe. Assuming current ‘concordance’ values for the cosmological parameters, we plot halo abundance against redshift as a function of halo mass, halo temperature, the fraction of cosmic matter in haloes, halo clustering strength, and the clustering strength of the z= 0 descendants of high-redshift haloes. These plots are useful for understanding how nonlinear structure grows in the model. They demonstrate a number of properties that may seem surprising, for example: 109 M⊙ haloes are as abundant at z= 20 as L* galaxies are today; 106 K haloes are equally abundant at z= 8 and at z= 0; 10 per cent of all matter is currently in haloes hotter than 1 keV, while more than half is in haloes too cool to trap photo-ionized gas; 1 per cent of all matter at z= 15 is in haloes hot enough to ionize hydrogen; haloes of given mass or temperature are more clustered at higher redshift; haloes with the abundance of present-day L* galaxies are equally clustered at all z < 20; the metals produced by star-formation at z > 10 are more clustered at z= 0 than are L* galaxies." @default.
- W2065201732 created "2016-06-24" @default.
- W2065201732 creator A5032581326 @default.
- W2065201732 creator A5079556845 @default.
- W2065201732 date "2002-10-01" @default.
- W2065201732 modified "2023-10-18" @default.
- W2065201732 title "The abundance and clustering of dark haloes in the standard ΛCDM cosmogony" @default.
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- W2065201732 doi "https://doi.org/10.1046/j.1365-8711.2002.05723.x" @default.
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