The Dispersion Velocity of Galactic Dark Matter Particles

Astronomy and Astrophysics – Astrophysics

Scientific paper

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RevTex, 4 pages, 1 ps figure, accepted for publication in Physical Review Letters

Scientific paper

10.1103/PhysRevLett.76.3886

The self-consistent spatial distribution of particles of Galactic dark matter
is derived including their own gravitational potential, as also that of the
visible matter of the Galaxy. In order to reproduce the observed rotation curve
of the Galaxy the value of the dispersion velocity of the dark matter
particles, $\rmsveldm$, should be $\sim 600\kmps$ or larger.

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