Modified Newtonian Dynamics: A Falsification of Cold Dark Matter
Author(s) -
R. H. Sanders
Publication year - 2009
Publication title -
advances in astronomy
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.364
H-Index - 34
eISSN - 1687-7977
pISSN - 1687-7969
DOI - 10.1155/2009/752439
Subject(s) - physics , modified newtonian dynamics , dark matter , galaxy rotation curve , astrophysics , cold dark matter , galaxy , newtonian dynamics , spiral galaxy , galaxy formation and evolution , theoretical physics
The only viable alternative to dark matter is one in which Newtonian dynamicsor gravity breaks down in the limit of low accelerations, as in modified Newtonian dynamics (MONDs). This hypothesis, suggested by Milgrom, has been successful in explaining systematic properties of spiral and elliptical galaxies and predicting in detail the observed rotation curves of spiral galaxies with only one additional parameter—a critical acceleration which is on the order of the cosmologically interesting value of . MOND may be viewed as an algorithm for calculating the distribution of force in an astronomical object from the observed distribution of baryonic matter. The fact that it works very well on the scale of galaxies is problematic for colddark matter (CDM). Here I present evidence in favor of this assertion and claim that this is, in effect, a falsification of CDM on the scale of galaxies
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