Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-08-02
Phys.Rev.D72:101301,2005
Astronomy and Astrophysics
Astrophysics
5 pages, 2 figures; v2 minor modifications to match version published as "Test of modified newtonian dynamics with recent Boom
Scientific paper
10.1103/PhysRevD.72.101301
Purely baryonic dark matter dominated models like MOND based on modification of Newtonian gravity have been successfully in reproducing some dynamical properties of galaxies. More recently, a relativistic formulation of MOND proposed by Bekenstein seems to agree with cosmological large scale structure formation. In this work, we revise the agreement of MOND with observations in light of the new results on the Cosmic Microwave Anisotropies provided by the 2003 flight of Boomerang. The measurements of the height of the third acoustic peak, provided by several small scale CMB experiments have reached enough sensitivity to severely constrain models without cold dark matter. Assuming that acoustic peak structure in the CMB is unchanged and that local measurements of the Hubble constant can be applied, we find that the cold dark matter is strongly favoured with Bayesian probability ratio of about one in two hundred.
Melchiorri Alessandro
Silk Joseph
Slosar Anze
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