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astro-ph1995
Redshift dependence of clustering in numerical simulations
Volker Mueller
High resolution -body simulations for variants of the CDM model are used to derive the redshift dependence of galaxy formation and of galaxy correlation functions. The reconstru…
astro-ph1995
SIMULATING LARGE-SCALE STRUCTURE FORMATION FOR BSI POWER SPECTRA
V. Mueller
A double inflationary model provides perturbation spectra with enhanced power at large scales (Broken Scale Invariant perturbations -- BSI), leading to a promising scenario for the…