MOND in the Early Universe

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.

arXiv commentContribution to '98 October conference, After the Dark Ages, eds. Smith & Holt, 4 pages

Cited by in corpus (4)

• A Tale of Two Paradigms: the Mutual Incommensurability of LCDM and MOND
• Confrontation of MOND Predictions with WMAP First Year Data
• Hydrodynamical structure formation in Milgromian cosmology
• Predictions for the sky-averaged depth of the 21cm absorption signal at high redshift in cosmologies with and without non-baryonic cold dark matter