In this thesis I test the modified Newtonian dynamics as an alternative to the colddark matter hypothesis. In the Milky Way, I show that the dynamics of the dwarf galaxies are well described by the paradigm and I confirm its distant low surface brightness globularclusters provide a strong test, for which I make predictions. Through analysis of a sample of 26 X-ray bright galaxy groups andclusters I demonstrate that the three active neutrinos and their anti-particles are insufficient to reconcilemodified Newtonian dynamics with the observed temperatures of the X-ray emitting gas, norwith weak-lensing measurements, in particular for the bullet cluster. To this end, I propose an 11eV sterile neutrino toserendipitously resolve the residual mass problem in X-ray bright groups and clusters,as well as matching the angular power spectrum of the Cosmic MicrowaveBackground. With this in mind, I show that the large collision velocity of the bullet cluster and the high number of colliding clusters is more naturally reproduced in MOND thanin standard dynamics.
【 预 览 】
附件列表
Files
Size
Format
View
Modified Newtonian dynamics at all astrophysical scales