ASTROPHYSICAL S-FACTOR OF 6 Li(p,γ) 7 Be REACTION FROM EXPERIMENTAL DATA USING DIFFERENT METHODS

N. Burtebayev; Zh. Kerimkulov; A. Amar; S. B. Dubovichenko; S. B. Sakuta; S. V. Artemov

ASTROPHYSICAL S-FACTOR OF 6 Li(p,γ) 7 Be REACTION FROM EXPERIMENTAL DATA USING DIFFERENT METHODS

Авторлар

N. Burtebayev Institute of Nuclear Physics of National Nuclear Center
Zh. Kerimkulov Institute of Nuclear Physics of National Nuclear Center
A. Amar Kazakh National University
S. B. Dubovichenko V. G. Fesenkov Аstrophysical Institute of NSRTC NSA of RK
S. B. Sakuta Russian Research Center “Kurchatov institute”
S. V. Artemov Institute of Nuclear Physics , Ядролық физика институты

Кілт сөздер:

ray transitions, a model using Fresco program

Аңдатпа

New measurements of the 6 Li(p,γ) 7 Be reaction γ-ray angular distributions have been done at beam energies of Ep, lab. = 387, 690, 984 and 1283 keV for the γ-ray transitions to the ground and first excited (1/2-, 429 keV) states in 7 Be. Our calculations of the cross section of the 6 Li (p, γ) 7 Be reaction was carried within the framework of the direct capture in the potential model using Fresco program. We extracted both of spectroscopic factors of 7 Be and astro S-factor 6 Li+p→7 Be+γ from experimental data using two different methods.

Жүктеулер

Журналдың саны

Нөмір 39 № 4 (2011): KazNU Bulletin. Physics series

Бөлім

Plasma Physics

Дәйексөзді қалай келтіруге болады

[1]

N. Burtebayev, Z. Kerimkulov, A. Amar, S. B. Dubovichenko, S. B. Sakuta, and S. V. Artemov, “ASTROPHYSICAL S-FACTOR OF 6 Li(p,γ) 7 Be REACTION FROM EXPERIMENTAL DATA USING DIFFERENT METHODS”, Rec.Contr.Phys., vol. 39, no. 4, pp. 40–50, Dec. 2011, Accessed: Aug. 17, 2026. Available: https://bph.kaznu.kz/index.php/zhuzhu/article/view/161