Journalartikel

From dinuclear systems to close binary stars: Application to source of energy in the universe


AutorenlisteSargsyan, V. V.; Lenske, H.; Adamian, G. G.; Antonenko, N., V

Jahr der Veröffentlichung2018

ZeitschriftInternational Journal of Modern Physics E

Bandnummer27

Heftnummer11

ISSN0218-3013

eISSN1793-6608

Open Access StatusGreen

DOI Linkhttps://doi.org/10.1142/S0218301318500933

VerlagWorld Scientific Publishing


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.



Zitierstile

Harvard-ZitierstilSargsyan, V., Lenske, H., Adamian, G. and Antonenko, N. (2018) From dinuclear systems to close binary stars: Application to source of energy in the universe, International Journal of Modern Physics E, 27(11), Article 1850093. https://doi.org/10.1142/S0218301318500933

APA-ZitierstilSargsyan, V., Lenske, H., Adamian, G., & Antonenko, N. (2018). From dinuclear systems to close binary stars: Application to source of energy in the universe. International Journal of Modern Physics E. 27(11), Article 1850093. https://doi.org/10.1142/S0218301318500933



Schlagwörter


Close binary starsmass asymmetrymass transfer


Nachhaltigkeitsbezüge


Zuletzt aktualisiert 2025-10-06 um 10:57