Abstract
Abstract The microlensing of the distant stars by neutralino stars is considered. The neutralino sars have been considered in the recent paper of Gurevich and Zybin; moreover, it has been suggested that the stars should be regard as a major component of dark matter. The optics of these gravitational microlenses, namely the gravitational lens equation, its solutions, increasing of images and critical and caustic curves are analysed by using a clear approximation. The set of model parameters is considered.
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