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

Authors

  • 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 image/svg+xml , Institute of Nuclear Physics image/svg+xml

Keywords:

ray transitions, a model using Fresco program

Abstract

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.

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Issue

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

Section

Plasma Physics

How to Cite

[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. 16, 2026. Available: https://bph.kaznu.kz/index.php/zhuzhu/article/view/161

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