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Evolution of Clustering and Bias in a Lambda-CDM Universe

Romeel Davé·Lars Hernquist·Neal Katz·David H. Weinberg
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Abstract

We determine the evolution from $z=3\to 0$ of the galaxy and mass correlation functions and bias factor in a $50h^{-1}$Mpc $Λ$CDM hydrodynamic simulation with $10h^{-1}$kpc resolution. The mass correlation function grows with time, but the galaxy correlation function shows little evolution and is well described by a power law. At early times, galaxies are biased traces of mass, with bias being higher on smaller scales. By z=0, galaxies trace the mass, and the bias shows little scale dependence.

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Romeel Davé, Lars Hernquist, Neal Katz, David H. Weinberg. 1999-10-12. Evolution of Clustering and Bias in a Lambda-CDM Universe. https://arxiv.org/abs/astro-ph/9910221

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