Issue |
EPJ Web of Conferences
Volume 109, 2016
The 13th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG2015)
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Article Number | 01001 | |
Number of page(s) | 8 | |
Section | Big Bang Cosmology and Primordial Nucleosynthesis | |
DOI | https://doi.org/10.1051/epjconf/201610901001 | |
Published online | 12 February 2016 |
https://doi.org/10.1051/epjconf/201610901001
Explosive Nuclear Burning in the pp-Chain Region and the Breakout Processes
1 RIKEN Nishina Center, 2-1 Hirosawa, Wako, 351-0198, Saitama, Japan
2 Institute of Modern Physics, CAS, Lanzhou, China
3 Center for Nuclear Study, University of Tokyo, 2-1 Hirosawa, Wako, 351-0198, Saitama, Japan
a Corresponding author: kubono@riken.jp
Published online: 12 February 2016
The nuclear reactions in the pp-chain region and on the breakout process from the pp-chain region under very high temperature conditions are reviewed, and some possibilities for experimental investigation are discussed. The reactions discussed could play an important role typically for the primordial nucleosynthesis and supernova nucleosynthesis. Specifically, I discuss here the reactions starting from the two key nuclei, 7Be and 7Li. The 7Be(n,α) reaction, which destroys 7Be, is considered to have a large impact to the primordial 7Li problem. Our recent estimate of the reaction rate indicates that the reaction rate can be about one order of magnitude smaller than the rate currently adopted, suggesting this channel has a minor effect for the 7Li problem. Under a proton-rich environment at high temperature like the νp-process, the 7Be(α,γ)11C(α,p)14N pathway is expected to play a majpr role for heavy element synthesis, comparable to the triple alpha process. These two reactions on the pathway were investigated by using low-energy, high-intensity RI beams of 7Be and 11C. The results support the theoretical prediction of heavy nucleus production at around mass 90-100 by the νp-process, where the anomalously abundant p-nuclei exist. The reactions on the breakout sequence of 7Li(n,γ)8Li(α,n)11B are also discussed which could paly a crucial role in nuetron-rich envirnments, like in the primirdial universe as well as the early stage of the r-process. The cross sections of the first step reaction 7Li(n,γ)8Li seems well confirmed, but the second step reaction 8Li(α,n)11B still is not well known yet, whose status of the study is discussed.
© Owned by the authors, published by EDP Sciences, 2016
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