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Dark matter （DM） is a form of matter necessary to account for gravitational effects observed in very large scale structures such as anomalies in the rotation of galaxies and the gravitational lensing of light by galaxy clusters that cannot be accounted for by the quantity of observed matter （Bertone et al. 2005）. In the standard cosmology model, dark matter, dark energy and normal matter constitute about 23%, 72% and 5% of the energy density of the universe,