Experimental Nuclear and High Energy Physics, Astrophysics and Cosmic Rays
Investigations are carried out in the fields of:
Experimental spectrum of protons emitted in forward and backward directions
from the reaction 197Au + 32S at 840 MeV. Decomposition is obtained with
Fermi-jet model calculations. (INRNE and HMI-Berlin collaboration, Cortesy
Prof. B.Botchev)
Elementary particle and nuclear physics at high energies with accelerators
for studying the interactions and fundamental properties of matter by the
help of experiments SPHERE ( JINR -Dubna), EXCHARM (Serpukhov) and L3,
OBELIX, CMS, COMPASS (CERN) and COSY-GEM (Julich)
Low-energy nuclear physics for study the structure of atomic nuclei using
neutrons and accelerated heavy ions with the aim to clarify the properties
of excited nuclear states and nuclear matter as well as the nature of nuclear
forces
Mechanisms of nuclear reactions induced by accelerated charged ions in
energy range from Coulomb barrier up to 100 MeV/A in order to establish
contributions of different mechanisms taking place
Astrophysics studying the nuclear and energy spectra of primary cosmic
rays and astrophysical objects as local sources of ultra-high energy gamma-quanta
Cosmic ray physics, elementary particles, astrophysics and astronomy as
well as participation in the design of the international experiment for
extensive showers AUGER on 5000 m2 for studying of the upper energetic
limit of cosmic rays.