THE JINA REACLIB DATABASE: ITS RECENT UPDATES AND IMPACT ON TYPE-I X-RAY BURSTS

被引:803
作者
Cyburt, Richard H. [1 ]
Amthor, A. Matthew [1 ,2 ]
Ferguson, Ryan [1 ,2 ]
Meisel, Zach [1 ,2 ]
Smith, Karl [1 ,2 ]
Warren, Scott [1 ,3 ]
Heger, Alexander [4 ]
Hoffman, R. D. [5 ]
Rauscher, Thomas [6 ]
Sakharuk, Alexander [1 ]
Schatz, Hendrik [1 ,2 ]
Thielemann, F. K. [6 ]
Wiescher, Michael [7 ]
机构
[1] Michigan State Univ, Natl Superconducting Cyclotron Lab, E Lansing, MI 48824 USA
[2] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA
[3] Michigan State Univ, Dept Elect & Comp Engn, E Lansing, MI 48824 USA
[4] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA
[5] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA
[6] Univ Basel, Dept Phys, CH-4056 Basel, Switzerland
[7] Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA
基金
美国国家科学基金会;
关键词
nuclear reactions; nucleosynthesis; abundances; X-rays: bursts; WEAK-INTERACTION RATES; INTERMEDIATE-MASS NUCLEI; THERMONUCLEAR REACTION-RATES; DRIP-LINE NUCLEI; RP-PROCESS; CROSS-SECTIONS; ALPHA-PROCESS; RICH NUCLEI; END-POINT; NUCLEOSYNTHESIS;
D O I
10.1088/0067-0049/189/1/240
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present results from the JINA REACLIB project, an ongoing effort to maintain a current and accurate library of thermonuclear reaction rates for astrophysical applications. Ongoing updates are transparently documented and version tracked, and any set of rates is publicly available and can be downloaded via a Web interface at http://groups.nscl.msu.edu/jina/reaclib/db/. We discuss here our library V1.0, a snapshot of recommended rates for stable and explosive hydrogen and helium burning. We show that the updated reaction rates lead to modest but significant changes in full network, one-dimensional X-ray burst model calculations, compared with calculations with previously used reaction rate sets. The late time behavior of X-ray burst light curves shows significant changes, suggesting that the previously found small discrepancies between model calculations and observations may be solved with a better understanding of the nuclear input. Our X-ray burst model calculations are intended to serve as a benchmark for future model comparisons and sensitivity studies, as the complete underlying nuclear physics is fully documented and publicly available.
引用
收藏
页码:240 / 252
页数:13
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