pith. sign in

arxiv: 1812.11338 · v1 · pith:3XWTDPIUnew · submitted 2018-12-29 · 🌌 astro-ph.SR

From Dinuclear Systems to Close Binary Stars: Application to Source of Energy in the Universe

classification 🌌 astro-ph.SR
keywords binaryenergystarsclosestaramountanalyzedapplication
0
0 comments X
read the original abstract

The evolution of close binary stars in mass asymmetry (transfer) coordinate is considered. The conditions for the formation of stable symmetric binary stars are analyzed. The role of symmetrization of asymmetric binary star in the transformation of potential energy into internal energy of star and the release of a large amount of energy is revealed.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.