Astrophysical S-factors for complete fusion reactions $^{12,13}\textrm{C}\,+\,^{12,13}$C

IF 2.6 3区物理与天体物理 Q2 PHYSICS, NUCLEAR

The European Physical Journal A Pub Date : 2024-09-11 DOI:10.1140/epja/s10050-024-01406-3

V. V. Sargsyan, G. G. Adamian, N. V. Antonenko

引用次数: 0

Abstract

Comparative analysis of the complete fusion reactions $^{12}\textrm{C}\, +\, ^{12}\textrm{C}, ^{12}\textrm{C}\, +\, ^{13}$C and $^{13}\textrm{C}\, +\, ^{13}$C at extremely low energies is performed using the Extended Quantum Diffusion Approach. The theoretical calculations are compared with the available experimental data, and the results are discussed for future experiments. The study reveals the presence of a maximum in the astrophysical S-factor for these reactions.

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完全聚变反应的天体物理 S 因子 $$^{12,13}\textrm{C}\,+\,^{12,13}$$ C

使用扩展量子扩散法对极低能量下的完全聚变反应（^{12}\textrm{C}\, +\, ^{12}\textrm{C}, ^{12}\textrm{C}\, +\, ^{13}）C 和（^{13}\textrm{C}\, +\, ^{13}）C 进行了比较分析。将理论计算结果与现有的实验数据进行了比较，并讨论了未来实验的结果。研究揭示了这些反应的天体物理 S 因子存在一个最大值。

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

The European Physical Journal A 物理-物理：核物理

CiteScore

5.00

自引率

18.50%

发文量

216

审稿时长

3-8 weeks

期刊介绍： Hadron Physics Hadron Structure Hadron Spectroscopy Hadronic and Electroweak Interactions of Hadrons Nonperturbative Approaches to QCD Phenomenological Approaches to Hadron Physics Nuclear and Quark Matter Heavy-Ion Collisions Phase Diagram of the Strong Interaction Hard Probes Quark-Gluon Plasma and Hadronic Matter Relativistic Transport and Hydrodynamics Compact Stars Nuclear Physics Nuclear Structure and Reactions Few-Body Systems Radioactive Beams Electroweak Interactions Nuclear Astrophysics Article Categories Letters (Open Access) Regular Articles New Tools and Techniques Reviews.

Astrophysical S-factors for complete fusion reactions \(^{12,13}\textrm{C}\,+\,^{12,13}\)C

Abstract