Abstract
The evolution of close binary cosmic objects in the mass-asymmetry coordinate is considered. Conditions for the formation of stable symmetric binary stars and galaxies are analyzed. The role of symmetrization of an asymmetric binary system in the transformation of the potential energy into the internal energy and in the release of a large amount of energy is explained.
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Funding
This study was supported in part by Russian Foundation for Basic Research (project no. 17-52-12015) and by Deutsche Forschungsgemeinschaft (DFG) (Le439/16).
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The work of V.V. Sargsyan was supported in part by Alexander von Humboldt Stiftung (Bonn).
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Sargsyan, V., Lenske, H., Adamian, G. et al. From Dinuclear Systems to Close Binary Stars and Galaxies. Phys. Atom. Nuclei 83, 60–68 (2020). https://doi.org/10.1134/S1063778820010135
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DOI: https://doi.org/10.1134/S1063778820010135