In this work the prospects of cosmic ray astronomy in general and possibilities for particles originating from the galactic center and active galactic nuclei are investigated numerically by integrating trajectories of incoming cosmic rays backwards in time, in different models of the galactic magnetic ?eld. In principle it is concluded that cosmic ray astronomy is possible for cosmic protons with energies of 10 EeV and above.
D.09 Tutoring for postgraduate students
COBISS.SI-ID: 1327099In Japanese center for particle physics research KEK the upgrade of the KEKB factory and the Belle experiment have started. The aim of the upgrade is to perform precision experiments in the decays of B mesons, which will allow us to probe the physics beyond SM. I presented the experimental endeavour in the R&D of the new SVD for the upgraded B factory.
B.03 Paper at an international scientific conference
COBISS.SI-ID: 1459707