Abstract

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, 7 Be and 7 Li. The 7 Be(n,α) reaction, which destroys 7 Be, is considered to have a large impact to the primordial 7 Li 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 7 Li problem. Under a proton-rich environment at high temperature like the νp-process, the 7 Be(α,γ) 11 C(α,p) 14 N 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 7 Be and 11 C. 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 7 Li(n,γ) 8 Li(α,n) 11 B 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 7 Li(n,γ) 8 Li seems well confirmed, but the second step reaction 8 Li(α,n) 11 B still is not well known yet, whose status of the study is discussed.

Highlights

  • 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

  • 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

  • There still is a possibility that this problem comes from unstudied, or not well studied nuclear reactions in the pp-chain region in the primordial nucleosynthesis, so much efforts have been made for many years in nuclear astrophysics

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Summary

The pp-Chain Region and the Breakout Process

Observation of elements is one of the keys for studying the evolution of the universe as well as various stellar phenomena. There are several efforts reported for these reactions, but almost none are known well yet Another interesting point for the nucleosynthesis at high temperature in the proton-rich nuclear region is that neutron-induced reactions will play an important role like in the Qp-process. Another interesting reactions for the primordial nucleosynthesis are those on the possible pathway of the breakout from the pp-chain region, 7Li(n,J)8Li(D,n)11B [12] These reactions play an important role in the early stage of the r-process, as will be discussed in sec. Under proton-rich, high temperature conditions like in the Qp-process in the very early epoch of type II supernovae, nuclear reaction chains that involve proton-rich nuclei Figure 2 Schematic nucleosynthetic flows at very are considered to be favourable like high temperatures in the pp-chain and breakout 7Be(D J)11C(D,p)14N, and 7Be(D p)10B(D p) 13C regions.

The Qp-process in type II supernovae
Fate of 7Be
Fate of 7Li
Findings
Summary
Full Text
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