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

Authors

  • N. Burtebayev Institute of Nuclear Physics of National Nuclear Center, Almaty, Kazakhstan
  • A. Amar Al-Farabi Kazakh National University, Kazakstan, Almaty
  • S.B. Dubovichenko V. G. Fesenkov Аstrophysical Institute of NSRTC NSA of RK, Almaty, Kazakhstan
  • S.B. Sakuta Russian Research Center “Kurchatov institute”, Moscow, Russia
  • S.V. Artemov Institute of Nuclear Physics, Tashkent, Uzbekistan
  • Zh. Kerimkulov Al-Farabi Kazakh National University, Kazakstan, Almaty

Keywords:

potential model, Fresco program, 6Li(p,γ)7Be reaction

Abstract

New measurements of the 6Li(p,γ)7Be 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 7Be. Our calculations of the cross section of the 6Li (p, γ)7Be reaction was carried within the framework of the direct capture in the potential model using Fresco program. We extracted both of spectroscopic factors of 7Be and astro S-factor 6Li+p→7Be+γ from experimental data using two different methods.

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Published

2011-12-20

Issue

Section

Theoretical Physics. Nuclear and Elementary Particle Physics. Astrophysics

How to Cite

ASTROPHYSICAL S-FACTOR OF 6Li(p,γ)7Be REACTION FROM EXPERIMENTAL DATA USING DIFFERENT METHODS. (2011). Recent Contributions to Physics, 2011(4), 40-50. https://bph.kaznu.kz/index.php/zhuzhu/article/view/663

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