In CDM models, the power spectrum determines everything about structure in the Universe. In particular, it leads to what people refer to as “bottom-up” and/or “hierarchical clustering.” To begin, note that the power spectrum P (k), which decreases at large k (small wavelength) is psychologically inferior to the scaled power spectrum ∆2(k) = (1/2π2)k3P (k). This latter quantity is monotonically ...