Microlensing with the Radioastron Space Telescope

Mathematics – Logic

Scientific paper

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Scientific paper

It is well-known that gravitational lensing is a powerful tool in the investigation of the distribution of matter, including that of dark matter (DM). Typical angular distances between images and typical time scales depend on the gravitational lens masses. For the of microlensing, angular distances between images or typical astrometric shifts are about 10-5 - 10-6 as. Such an angular resolution will be reached with the space-ground VLBI interferometer, Radioastron. The basic targets for microlensing searches should be b point like images of gravitationally lensed systems and bright point-like radio sources at cosmological distances. In this case, an analysis of their variability and a solid determination of microlensing could lead to an estimation of their cosmological mass density.

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