Retrieving "Expansion Rate" from the archives
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Matter Energy Density
Linked via "expansion rate"
Cosmic Microwave Background (CMB): Anisotropies in the CMB power spectrum (especially the height of the first acoustic peak) directly constrain the total spatial curvature\} ($\Omegak$), which, assuming flatness ($\Omegak=0$), constrains $\Omegab + \Omegac + \Omega_{\Lambda} = 1$.
Baryon Acoustic Oscillations (BAO): The characteristic scale imprinted in galaxy clustering provides a "standard ruler" to measure the [expansion history](/entries/expan…