We study the capture of galactic dark matter particles (DMP) in two-body and
few-body systems with a symplectic map description. This approach allows
modeling the scattering of 1016 DMPs after following the time evolution of
the captured particle on about 109 orbital periods of the binary system. We
obtain the DMP density distribution inside such systems and determine the
enhancement factor of their density in a center vicinity compared to its
galactic value as a function of the mass ratio of the bodies and the ratio of
the body velocity to the velocity of the galactic DMP wind. We find that the
enhancement factor can be on the order of tens of thousands.Comment: 6 pages, 9 figure