ASTROPARTICLE PHYSICS - PRESENT AND FUTURE

The solar neutrinos, next SN and the dark matter are reviewed and analyzed from the point of view of future observations. For solar neutrinos much attention is given to an astrophysical solution of the problem. It is shown to be excluded unless the nuCl-37-cross-section is considerably underestimated or unless there are large systematic errors in the Homestake or Kamiokande experiments. For the next SN the main emphasis is made on the time-sequence of phenomena and on the possibilities of their observations. The neutralinos and neutrinos are discussed as the dark matter components for the Mixed Dark Matter model.