The astrophysical S factor of p+9Be radiative capture reaction in a potential model

IF 1.9 4区物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS

New Astronomy Pub Date : 2023-12-15 DOI:10.1016/j.newast.2023.102178

Leila Asgari, Hossein Sadeghi, Hassan Khalili

引用次数: 0

Abstract

In this work, we calculate the S-factor for $p +$ ⁹Be Radiative Capture Reaction according to a modified potential model. We consider the sum of all possible electrical and magnetic transitions as a total cross-section. The zero-energy $S$ -factor results are in good agreement with previously theoretical studies and the experimentally reported data.

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潜在模型中 p+9Be 辐射俘获反应的天体物理 S 因子

在这项工作中，我们根据修正的电位模型计算了p+9Be辐射捕获反应的s因子。我们把所有可能的电跃迁和磁跃迁的总和看作一个总横截面。零能量s因子的结果与先前的理论研究和实验报告的数据吻合得很好。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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来源期刊

New Astronomy 地学天文-天文与天体物理

CiteScore

4.00

自引率

10.00%

发文量

109

审稿时长

13.6 weeks

期刊介绍： New Astronomy publishes articles in all fields of astronomy and astrophysics, with a particular focus on computational astronomy: mathematical and astronomy techniques and methodology, simulations, modelling and numerical results and computational techniques in instrumentation. New Astronomy includes full length research articles and review articles. The journal covers solar, stellar, galactic and extragalactic astronomy and astrophysics. It reports on original research in all wavelength bands, ranging from radio to gamma-ray.