A New Estimate for the Dispersion Velocity of Galactic Dark Matter Particles

Physics

Scientific paper

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Scientific paper

An independent method is proposed to estimate the dispersion velocity of galactic dark matter particles. This method is based on the observed quasar-galaxy association samples that are caused by gravitational lensing. All resulting dispersion velocities are much higher than similar 220 km·s-1, a value expected from the virial theorem, which shows that the conventional assumption of virialization may be invalid in the halo regions of galaxies.

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