From Dinuclear Systems to Close Binary Stars: Application to Mass Transfer; Acta Physica Polonica B; Vol. 50, iss. 3
| Parent link: | Acta Physica Polonica B: Journal Vol. 50, iss. 3.— 2019.— [P. 507-516] |
|---|---|
| Corporate Author: | |
| Other Authors: | , , , |
| Summary: | Title screen 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. |
| Language: | English |
| Published: |
2019
|
| Subjects: | |
| Online Access: | https://doi.org/10.5506/APhysPolB.50.507 |
| Format: | Electronic Book Chapter |
| KOHA link: | https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=665299 |
MARC
| LEADER | 00000naa0a2200000 4500 | ||
|---|---|---|---|
| 001 | 665299 | ||
| 005 | 20250826112802.0 | ||
| 035 | |a (RuTPU)RU\TPU\network\36498 | ||
| 035 | |a RU\TPU\network\20555 | ||
| 090 | |a 665299 | ||
| 100 | |a 20210909d2019 k||y0rusy50 ba | ||
| 101 | 0 | |a eng | |
| 102 | |a PL | ||
| 135 | |a drcn ---uucaa | ||
| 181 | 0 | |a i | |
| 182 | 0 | |a b | |
| 200 | 1 | |a From Dinuclear Systems to Close Binary Stars: Application to Mass Transfer |f V. V. Sargsyan, H. Lenske, G. G. Adamyan, N. V. Antonenko | |
| 203 | |a Text |c electronic | ||
| 300 | |a Title screen | ||
| 320 | |a [References: 7 tit.] | ||
| 330 | |a 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. | ||
| 461 | |t Acta Physica Polonica B |o Journal | ||
| 463 | |t Vol. 50, iss. 3 |v [P. 507-516] |d 2019 | ||
| 610 | 1 | |a электронный ресурс | |
| 610 | 1 | |a труды учёных ТПУ | |
| 610 | 1 | |a двойные звезды | |
| 610 | 1 | |a массоперенос | |
| 610 | 1 | |a внутренняя энергия | |
| 610 | 1 | |a ядерная физика | |
| 701 | 1 | |a Sargsyan |b V. V. |g Vazgen Valerikovich | |
| 701 | 1 | |a Lenske |b H. |g Horst | |
| 701 | 1 | |a Adamyan |b G. G. |g Gurgen Grigorjevich | |
| 701 | 1 | |a Antonenko |b N. V. |c physicist |c Professor of Tomsk Polytechnic University, Doctor of physical and mathematical sciences |f 1964- |g Nikolay Viktorovich |3 (RuTPU)RU\TPU\pers\35905 |9 19046 | |
| 712 | 0 | 2 | |a Национальный исследовательский Томский политехнический университет (ТПУ) |b Физико-технический институт (ФТИ) |b Кафедра высшей математики и математической физики (ВММФ) |3 (RuTPU)RU\TPU\col\18727 |
| 801 | 2 | |a RU |b 63413507 |c 20210909 |g RCR | |
| 856 | 4 | |u https://doi.org/10.5506/APhysPolB.50.507 | |
| 942 | |c CF | ||