New nuclear physics for big bang nucleosynthesis

被引:56
|
作者
Boyd, Richard N. [1 ]
Brune, Carl R. [2 ]
Fuller, George M. [3 ]
Smith, Christel J. [4 ]
机构
[1] Lawrence Livermore Natl Lab, Livermore, CA 94551 USA
[2] Ohio Univ, Dept Phys & Astron, Athens, OH 45701 USA
[3] Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USA
[4] Arizona State Univ, Dept Phys, Tempe, AZ 85287 USA
来源
PHYSICAL REVIEW D | 2010年 / 82卷 / 10期
基金
美国国家科学基金会;
关键词
PROBE WMAP OBSERVATIONS; PRIMORDIAL NUCLEOSYNTHESIS; LI-6; PRODUCTION; CROSS-SECTIONS; DEUTERIUM; ABUNDANCE; HYDROGEN; LITHIUM; RATIO; PREDICTIONS;
D O I
10.1103/PhysRevD.82.105005
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss nuclear reactions which could play a role in big bang nucleosynthesis. Most of these reactions involve lithium and beryllium isotopes and the rates for some of these have not previously been included in BBN calculations. Few of these reactions are well studied in the laboratory. We also discuss novel effects in these reactions, including thermal population of nuclear target states, resonant enhancement, and nonthermal neutron reaction products. We perform sensitivity studies which show that even given considerable nuclear physics uncertainties, most of these nuclear reactions have minimal leverage on the standard BBN abundance yields of Li-6 and Li-7. Although a few have the potential to alter the yields significantly, we argue that this is unlikely.
引用
收藏
页数:12
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