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Nuclear reaction rate databases serve as essential inputs for nucleosynthesis and stellar evolution modeling, directly influencing the accuracy and physical reliability of calculations in various nuclear astrophysics processes. This work provides a comprehensive review of the major reaction rate databases—REACLIB, STARLIB, and BRUSLIB—highlighting their objectives, data structures, and representative applications, and discussing their coverage, fitting methods, and uncertainty evaluation. These databases have been instrumental in advancing the standardization of nuclear reaction network calculations. However, although these databases have significantly lowered the barrier to performing network modeling, there remains substantial room for improvement in aspects such as database unit structures, update mechanisms, and organizational frameworks. For example, detailed information on the underlying nuclear physics experiments or data analyses is often not included in REACLIB. Therefore, enhancing the stored metadata warrants careful consideration, since it can significantly improve the reliability of astrophysical modeling. At the same time, the advancement of nuclear astrophysics reaction rate databases depends heavily on continuous progress at the experimental frontier. In recent years, innovative experimental techniques—such as novel 4π high-resolution detector arrays and γ–charged particle coincidence measurements—have been widely applied to studies of key nuclear astrophysics reactions, significantly expanding research capabilities. To meet the demands of cutting-edge astrophysical studies for accurate reaction rates, the real-time updating and systematic evaluation of experimental data for key reactions represent both an important opportunity and an urgent challenge for the development of modern databases. several important achievements of the JUNA Collaboration at the Jinping underground nuclear astrophysics facility, where low-background experiments have been conducted, are also presented in this paper. These new low-energy measurements, when compared with traditional extrapolations used in databases, are found to provide more direct constraints on key reactions in nuclear astrophysics and to offer crucial experimental support for the continuous optimization of future databases.
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Keywords:
- nuclear astrophysics /
- nuclear reaction rate database /
- stellar nucleosynthesis /
- underground experiment
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图 1 核天体物理与其他主要物理学领域之间可能联系的示意图展示
Figure 1. Diagrammatic presentation of possible connections of nuclear astrophysics with other major fields of physics.
图 4 12C+12C熔合反应天体物理$ S^* $因子. TTIK实验[61]、数据库编评数据[22]、特洛伊木马方法(THM)实验数据[63], 反对称分子动力学模型计算结果分别用红色实线, 深蓝色点划线, 黑色虚线, 淡蓝色点划线表示
Figure 4. Astrophysical S-factor of the $ ^{12}\mathrm{C}+{}^{12}\mathrm{C} $ fusion reaction. The results from TTIK experiments[61], evaluated database data[22], Trojan Horse Method (THM) experimental data[63], and antisymmetrized molecular dynamics (AMD) calculations are represented by the red solid line, dark blue dash-dotted line, black dashed line, and light blue dash-dotted line, respectively.
表 1 三种主要核反应率数据库的表达方式与特点
Table 1. XXXXXXXXXXX
数据库 数据格式 数据库特点 REACLIB 七参数解析表达式 解析形式统一, 适用于大规模恒星演化与核合成网络(如XNet[33]、
MESA[34]、Kepler[35]); 通常不直接提供反应率不确定度信息.BRUSLIB 表格化(温度vs核反应率) 包含基于实验的汇编(如NACRE/NACREII)与大规模Hauser-Feshbach(HF)预测
两部分; 在质量数>40, 且位于接近稳定核素带区域的复合核研究中更为可靠[15].STARLIB 表格化(温度vs核反应率
vs反应不确定度)提供特定温度下每个反应率的概率密度函数, 严格定义反应率
不确定度[29], 便于开展核反应的蒙特卡洛全局敏感度分析[16].
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表 3 近年来若干核天体物理关键核反应实验测量及数据库收录
Table 3. XXXXXXXXX
核反应 实验技术 核反应率数据库收录 参考文献 25Mg(p, γ)26Al 地下实验直接测量 REACLIB未更新 [79] 13C(α, n)16O 地下实验直接测量 REACLIB未更新 [76,80] 19F(p, γ)20Ne 地下实验直接测量 REACLIB未更新 [81] 19F(p, α)16O 地下实验直接测量 REACLIB未更新 [82] 18O(α, γ)22Ne 地下实验直接测量 REACLIB未更新 [77,83] 2H(p, γ)3He 地下实验直接测量 REACLIB未更新 [71] 12, 13C(p, γ)13, 14N 地下实验直接测量 REACLIB未更新 [73] 59Fe(n, γ)60Fe β-Oslo方法 REACLIB未更新 [52] 22Mg(α, p)25Al MUSIC, AT-TPC REACLIB未更新 [56,85] 14C(n, γ)15C 超导螺线管 REACLIB未更新 [59] 12C+12C THM, TTIK REACLIB未更新 [61,63] 12C(α, γ)16O ANC REACLIB未更新 [86,87] 22Ne(α, n)25Mg, 22Ne(α, γ)26Mg 转移反应, 直接测量 REACLIB未更新 [88] 39K(p, γ)40Ca 转移反应 STARLIB, REACLIB [89] 18Ne(α, p)21Na 镜像核, 转移反应 STARLIB [90] 9Be(n, γ)10Be 活化法+AMS REACLIB [91] 30Si(p, γ)31P 直接测量 REACLIB [92]
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