MOND in the Early Universe
classification
🌌 astro-ph
gr-qchep-ph
keywords
mondappearbackgroundbaryonclustersconsequencescosmologydistinguishing
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I explore some consequences of Milgrom's modified dynamics for cosmology. There appear to be two promising tests for distinguishing MOND from CDM: (1) the rate of growth of structure and (2) the baryon fraction. These should be testable with observations of clusters at high redshift and the microwave background, respectively.
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