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23 April 2024
 
  » arxiv » astro-ph/9910221

 Article overview


Evolution of Clustering and Bias in a Lambda-CDM Universe
Romeel Davé ; Lars Hernquist ; Neal Katz ; David H. Weinberg ;
Date 12 Oct 1999
Subject astro-ph
AffiliationPrinceton), Lars Hernquist (CfA), Neal Katz (UMass), David H. Weinberg (Ohio State
AbstractWe determine the evolution from $z=3 o 0$ of the galaxy and mass correlation functions and bias factor in a $50h^{-1}$Mpc $Lambda$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.
Source arXiv, astro-ph/9910221
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