Konferenzpaper

Jahr der Veröffentlichung: 2019

Seiten: 507-516

Zeitschrift: Acta Physica Polonica B

Bandnummer: 50

Heftnummer: 3

ISSN: 0587-4254

eISSN: 1509-5770

Open Access Status: Bronze

DOI Link: https://doi.org/10.5506/APhysPolB.50.507

Konferenz: Zakopane Conference on Nuclear Physics - Extremes of the Nuclear Landscape

Verlag: Jagiellonian University

Abstract: 
Applying the microscopic nuclear physics ideas to macroscopic stellar systems, we study the evolution of the compact di-stars in mass asymmetry (transfer) coordinate. Depending on the internal structure of constituent stars, the initial mass asymmetry, total mass, and orbital angular momentum, the close di-star system can either exist in symmetric configuration or fuse into mono-star. The limitations 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 binary star and the release of a large amount of energy is revealed.

Harvard-Zitierstil: Sargsyan, V., Lenske, H., Adamian, G. and Antonenko, N. (2019) FROM DINUCLEAR SYSTEMS TO CLOSE BINARY STARS: APPLICATION TO MASS TRANSFER, Acta Physica Polonica B, 50(3), pp. 507-516. https://doi.org/10.5506/APhysPolB.50.507

APA-Zitierstil: Sargsyan, V., Lenske, H., Adamian, G., & Antonenko, N. (2019). FROM DINUCLEAR SYSTEMS TO CLOSE BINARY STARS: APPLICATION TO MASS TRANSFER. Acta Physica Polonica B. 50(3), 507-516. https://doi.org/10.5506/APhysPolB.50.507