MOND in the Early Universe
arXiv:astro-ph/9812328 · doi:10.1063/1.58637
Abstract
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.
Contribution to '98 October conference, After the Dark Ages, eds. Smith & Holt, 4 pages