Physics – Nuclear Physics – Nuclear Theory
Scientific paper
2010-12-08
Physics
Nuclear Physics
Nuclear Theory
280 p
Scientific paper
The book examines some of the questions of modern cosmology, the physics of atmospheric phenomena, the physics of quasi-particles and atomic nuclei in the Universe. It consists of three parts, each discusses the theoretical problems of various subjects of cosmic physics. The first part examines the physics of the expanding Universe, with emphasis on the content of the latest revolution in cosmology. It is today well established that the universe is dominated by a vacuum that exceeds the density of baryonic forms of cosmic matter, that the dynamics of the cosmic expansion controls the vacuum antigravity and, finally, that the cosmological expansion is accelerating. In the second part we investigate the processes leading to the electrization of gas fluxes in the solar atmosphere and the generation of neutrons in the active regions of its atmosphere, issues of electrization of thunderstorm clouds in the troposphere of the Earth, the formation and development of noctilucent clouds in the area of the mesosphere. In the third part the methods of calculating the wave functions of cluster systems in continuous and discrete spectrum for a given intercluster interaction are proposed. It presents the theoretical study of astrophysical S-factors in the photonuclear reactions, which are part of the helium thermonuclear processes cycle which determine the bulk of the energy yield in stellar systems. Although the book is written in Russian, it might have some interest.
Chechin L. M.
Dubovichenko S. B.
Takibaev N. Zh.
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