Stacy McGaugh
Published 1998-12-17Version 1
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.
Comments: Contribution to '98 October conference, After the Dark Ages, eds. Smith & Holt, 4 pages
Varying $α$ in the early universe: CMB, LSS and FMA
Physics of the Very Early Universe
Metallicity Evolution in the Early Universe
