http://arxiv.org/abs/1905.09821
Applying the microscopic nuclear physics ideas for fusion reactions to macroscopic galactic systems, we study the evolution of the compact binary galaxy in mass asymmetry (transfer) coordinate. The conditions for the formation of stable symmetric binary galaxy are analyzed. The role of symmetrization of asymmetric binary galaxy in the transformation of gravitational energy into internal energy of galaxies accompanied by the release of a large amount of energy during the symmetrization process is revealed.
V. Sargsyan, H. Lenske, G. Adamian, et. al.
Mon, 27 May 19
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Comments: arXiv admin note: text overlap with arXiv:1812.11338
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