Study on the Reaction Rate of Key Reaction $\bf ^{12}$C($\bm\upalpha$,~$\bm\upgamma$)$\bf ^{16}$O in Astrophysics Base on Shanghai Laser Electron $\bm\upgamma$ Source

XU Yi; XU Wang; MA Yu-Gang; CAI Xiang-Zhou; CHEN Jin-Gen; GU Jia-Hui; GUO Wei; PAN Qiang-Yan; SHEN Wen-Qing; WANG Cheng-Bin; WANG Hong-Wei; XU Jia-Qiang; YUAN Ren-Yong

Chinese Physics C> 2006, Vol. 30> Issue(S2) : 252-254

Study on the Reaction Rate of Key Reaction $\bf ^{12}$C($\bm\upalpha$,~$\bm\upgamma$)$\bf ^{16}$O in Astrophysics Base on Shanghai Laser Electron $\bm\upgamma$ Source

Shanghai Institute of Applied Physics, CAS, Shanghai 201800, China

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The MeV photon beam will be produced by Shanghai Laser Electron γ Source which is being proposed. Based on it, a series of nuclear astrophysics experiments can be carried on and the reaction rates of these reactions can be determined accurately. In this paper, the reaction rates of the key reaction ¹²C(α,γ)¹⁶O are calculated according to experiments data and theoretical results, and the mean value and statistical error of these calculated rates are evaluated. The new set of parameters of reaction rate formula are obtained though fitting above results. The reaction rate and its error at T₉=0.2 in which ¹²C(α,γ)¹⁶O occurred are extracted, and the screening effects of reaction rate are discussed.

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XU Yi, XU Wang, MA Yu-Gang, CAI Xiang-Zhou, CHEN Jin-Gen, GU Jia-Hui, GUO Wei, PAN Qiang-Yan, SHEN Wen-Qing, WANG Cheng-Bin, WANG Hong-Wei, XU Jia-Qiang and YUAN Ren-Yong. Study on the Reaction Rate of Key Reaction $\bf ^{12}$C($\bm\upalpha$,~$\bm\upgamma$)$\bf ^{16}$O in Astrophysics Base on Shanghai Laser Electron $\bm\upgamma$ Source[J]. Chinese Physics C, 2006, 30(S2): 252-254.

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Received: 2006-10-18
Revised: 1900-01-01

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通讯作者: 陈斌, [email protected]

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沈阳化工大学材料科学与工程学院沈阳 110142

Study on the Reaction Rate of Key Reaction $\bf ^{12}$C($\bm\upalpha$,~$\bm\upgamma$)$\bf ^{16}$O in Astrophysics Base on Shanghai Laser Electron $\bm\upgamma$ Source

Corresponding author: XU Yi,

Shanghai Institute of Applied Physics, CAS, Shanghai 201800, China

Received Date: 2006-10-18

Accepted Date: 1900-01-01

Available Online: 2006-01-03

Abstract: The MeV photon beam will be produced by Shanghai Laser Electron γ Source which is being proposed. Based on it, a series of nuclear astrophysics experiments can be carried on and the reaction rates of these reactions can be determined accurately. In this paper, the reaction rates of the key reaction ¹²C(α,γ)¹⁶O are calculated according to experiments data and theoretical results, and the mean value and statistical error of these calculated rates are evaluated. The new set of parameters of reaction rate formula are obtained though fitting above results. The reaction rate and its error at T₉=0.2 in which ¹²C(α,γ)¹⁶O occurred are extracted, and the screening effects of reaction rate are discussed.

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Study on the Reaction Rate of Key Reaction $\bf ^{12}$C($\bm\upalpha$,~$\bm\upgamma$)$\bf ^{16}$O in Astrophysics Base on Shanghai Laser Electron $\bm\upgamma$ Source

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