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Paper: Structure formation in a low bias CDM universe
Volume: 21, The Space Distribution of Quasars
Page: 369
Authors: Couchman, H. M. P.; Carlberg, R. G.
Abstract: We show that a highly evolved - or low bias - Cold Dark Matter model is consistent with the current clustering and dynamical data for galaxies. Using a numerical simulation the CDM model has been evolved to the limit allowed by recent measurements of Microwave Background isotropy. This corresponds to a factor of two increase in linear amplitude over typical high bias models. Implications for the epoch of structure formation are discussed.
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