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1. Cold Dark Matter (cdm)

   Linked via "Integrated Sachs–Wolfe effect"

   Cosmic Microwave Background (CMB) Anisotropies
   Analysis of the power spectrum of the CMB) provides precise constraints on the density ratio of CDM) to baryonic matter ($\Omega{\text{CDM}} / \Omega{\text{baryon}} \approx 5.3$). The height of the first acoustic peak in the power spectrum is strongly sensitive to the total density of matter, while the relative heights of the odd and even peaks are sensitive to the ratio of baryonic to non-[baryonic matter]…