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Nuclear Astrophysics Experiments in Collaboration with Ruhr University
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作者 曾晟 F. RAIOLA +4 位作者 T. SPILLANE 连刚 王宝祥 颜胜权 c. rolfs 《Plasma Science and Technology》 SCIE EI CAS CSCD 2012年第6期492-495,共4页
This paper reports on two nuclear astrophysics experiments performed in collabora- tion with Ruhr University. In a 12C+2C fusion reaction, the 12C(12C, a)20e and 12C(12C, p)23Na reactions were studied in the ener... This paper reports on two nuclear astrophysics experiments performed in collabora- tion with Ruhr University. In a 12C+2C fusion reaction, the 12C(12C, a)20e and 12C(12C, p)23Na reactions were studied in the energy range of E = 2.10 MeV to 4.75 MeV using -y-ray spectroscopy. The deduced astrophysical S(E)* factor exhibited a new, strong resonance at E -= 2.14 MeV, which lay at the high-energy tail of the Gamow peak. The resonance increased the reaction rate of the ^-channel by a factor of five near T = 8 ~ l0s K. The electron screening in d(d, p)t was stud- ied for a series of deuterated metal, insulator and semiconductor targets. Compared with the measurements performed with a gaseous D2 target, a large effect was observed in most metals, while a comparatively small effect was found in the insulators and semiconductors. Subsequently the temperature dependence of the electron screening in the d(d, p)t reaction was studied for the deuterated metals Pt and Co. Enhanced electron screening decreased with increasing tempera- ture. These data represent the first observations of the temperature dependence of a nuclear cross section. 展开更多
关键词 nuclear astrophysics 12C+12C fusion reaction direct measurement electron screening
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