THE DEFLECTION OF LIGHT RAYS IN THE GALAXIES’ HALOS OF DARK MATTER
Abstract
The deflection of light rays in the halos of dark matter described by Navarro-Frenk-White, Burket, Einasto and Kravtsov-Klypin profiles were searched. Numerical estimations for deflecting angles gives magnitude ~0.”00001, that are two orders smaller than achievement accuracy at the gravitational microlensing.
