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Information × Registration Number 0222U003453, 0119U100311 , R & D reports Title Investigation of fundamental problems of neutrino physics, cosmomicrophysics and nuclear physics. popup.stage_title Head Kadenko Igor M., Доктор фізико-математичних наук Registration Date 24-03-2022 Organization Taras Shevchenko National University of Kyiv popup.description2 Object of research: Neutrinos, high-energy neutrino fluxes, baryon asymmetry of the universe, neutrino oscillations, black holes, high-energy inelastic scattering of particles, atomic nucleus, cross sections of nuclear reactions. Purpose: to develop a set of programs for research astrophic processes on the DUNE detector and modeling of physical processes involving neutrinos in supernovae and for the DUNE neutrino experiment. The study of the generation of magnetic fields in models of the early universe with chirically disturbed anomalies and the study of tensor-scalar relations and spectral indices in cosmological models inflation with slow jumping and the study of the manifestations of superconducting space (super) strings as sources of collimated fluxes of high-energy neutrinos, the study of the process of birth of particles from vacuum in terms of the Unru effect. Investigations of photon force functions (FSF) taking into account the low energy states of the nucleus and experimental study of cross sections of nuclear reactions in the interaction with neutrons on neutron generators. Research methods: the use of nuclear-physical complexes equipment and models for describing nuclear reactions, and the interaction of gamma quanta and neutrons with nuclei. Modeling of physical processes with the participation of neutrinos in supernovae and the use of the neutrino experiment DUNE as an effective tool of neutrino astronomy for the study of supernova physics. The observations of collimated neutrino fluxes of ultrahigh energies from casps on superconducting space strings were observed by LOFAR, SKA 24 radio detectors and the JEM-EUSO space mission. Analytical expressions for E1, E2 and M1 photon force functions (FSF) tested and confirmed taking into account the FSF amplification due to the effects of the nucleus structure (presence of low-energy states), as well as according to the presence amplification factor between response function and FSF in heated nuclei.  Product Description popup.authors Bezshyiko Oleg A. Buhayev Kyrylo О. Golinka-Bezshyyko Larisa O. Horbachenko Oleksandr М. Dzysiuk Nataliia R. Dozenko Ivan S. Zadorozhna Lidiia V. Kadenko Artem О. Kolesnyk Oleksandr S. Kryachok Kateryna О. Lyubarska Mariya V. Ostapchuk Oksana A. Petrenko Vitaliy М. Plyuyko Volodymyr A. Siedov Yurii O. Solodovnyk Kateryna M. Tarakanov Valerii K. Teslik Olena М. popup.nrat_date 2022-03-24 Close