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Isobar-analogue reactions <sup>6</sup>Li(p,γ)<sup>7</sup>Be and <sup>6</sup>Li(n,γ)<sup>7</sup>Li relevant to the <sup>6</sup>Li/<sup>7</sup>Li ratio

ORAL

Abstract

In the framework of the modified potential cluster model with forbidden states formulated in [1] the isobar-analogue 6Li(p,γ)7Be and 6Li(n,γ)7Li reactions in the temperature range from 0.01 to 10 T9 are studied. While the dominant sources that determine the 6Li/7Li ratio are 4He(d,γ)6Li and 4He(t,γ)7Li processes, a qualitative feature of the reactions of radiative capture of neutrons 6Li(n,γ)7Li and protons 6Li(p,γ)7Be(e-ν)7Li can lead to a redistribution of lithium isotopes in the 6Li/7Li balance. These reactions are included in the calculations of the mass fractions as “destructive” for the 6Li isotope. The contribution of the isobar-analogue 6Li(p,γ)7Be and 6Li(n,γ)7Li reactions into the 6Li/7Li balance is estimated from the corresponding rates of these processes, the astrophysical S-factor for 6Li(p,γ)7Be is calculated and compared with the available experimental data and calculations done within different models. Cross-sections for 6Li(p,γ)7Be and 6Li(n,γ)7Li calculated using [1] are in reasonable agreement with experimental data.



[1] S. B. Dubovichenko, A. S. Tkachenko, R. Ya. Kezerashvili, N. A. Burkova, A. V. Dzhazairov-Kakhramanov, Phys. Rev. C 105, 065806, 2022.

Publication: S. B. Dubovichenko, A. S. Tkachenko, R. Ya. Kezerashvili, N. A. Burkova, A. V. Dzhazairov-Kakhramanov, Phys. Rev. C 105, 065806, 2022.

Presenters

  • Alessya S Tkachenko

    Fesenkov Astrophysical Institute, Almaty, Kazakhstan

Authors

  • Alessya S Tkachenko

    Fesenkov Astrophysical Institute, Almaty, Kazakhstan

  • Nataliya A Burkova

    al-Farabi Kazakh National University, Almaty, Kazakhstan

  • Sergey B Dubovichenko

    Fesenkov Astrophysical Institute, Almaty, Kazakhstan

  • Roman Y Kezerashvili

    The Graduate Center, City University of New York