The nature of dark matter and galactic rotation curves

Physics

Scientific paper

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Dark Matter, Kinematics, Dynamics, And Rotation, Background Radiations

Scientific paper

It is shown that if dark matter consists of particles of masses mi, spins Ji then mi=2kT/v2m=156.9E-1/4 keV (vm is the galactic rotation velocity at large r and T is the temperature of dark matter at the galactic location, E is the emissivity of dark matter at 6450 angstroms. Relations determining the emissivity of dark matter and the flux of radiation originating in a halo of dark matter are given [Eqs. (7), (8)].

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