Analysis of cross-section, S-factor and thermonuclear reaction rate of 8Li(α,n)11B and 14N(p,γ)15O using TALYS and EMPIRE nuclear reaction codes

Author:

Mondal Satabdi1,Das Pampa2,Senapati Enakshi1,Pandit Deepak3,Dey Balaram1,De Alokkumar4,Bhattacharya Srijit5

Affiliation:

1. Department of Physics, Bankura University, Bankura 722155 WB, India

2. Department of Physics, West Bengal State University, Barasat, Kolkata 700126 WB, India

3. Variable Energy Cyclotron Center, 1/AF-Bidhannagar, Kolkata 700064 WB, India

4. Department of Physics, Raniganj Girls’ College, Raniganj, 713358 WB, India

5. Department of Physics, Barasat Government College, Barasat, Kolkata 700124 WB, India

Abstract

Theoretical nuclear reaction codes are crucial for studying cross-section and S-factors of nuclear reactions required for the thermonuclear reaction rate calculations. We analyze two reactions 8Li([Formula: see text])11B and 14N([Formula: see text])15O, using both TALYS and EMPIRE codes. We stress that these reactions are highly important for CNO cycle but the extent of involvement of experimental datasets are meager and conflicting. For the first reaction, the trend of experimental data has been predicted satisfactorily by the codes. The reaction rate is also matched with REACLIB calculation. However, in 14N([Formula: see text])15O, none of the codes could predict the resonant structures in the experimental data at the lower energies. The importance of our work is a sincere attempt to validate the TALYS and EMPIRE predictions for cross-section, S-factor and the reaction rate, simultaneously.

Publisher

World Scientific Pub Co Pte Ltd

Subject

General Physics and Astronomy,Nuclear and High Energy Physics

Cited by 1 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. The reaction rate of radiative n8Li capture in the range from 0.01 to 10 T9;Frontiers in Astronomy and Space Sciences;2023-09-01

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