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New direct measurement of the ~6Li(p,γ)~7Be cross section at LUNA

机译:Luna的〜6Li(p,γ)〜7be横截面的新直接测量

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The ~6Li(p,γ)~7Be reaction is involved in many astrophysical scenario, ranging from Big Bang Nucleosynthesis to pre-main sequence stellar evolution and solar neutrino. At astrophysical energies, proton capture on ~6Li proceeds through the ~6Li(p,α)~3He and the ~6Li(p,γ)~7Be reactions. A recent measurement of the ~6Li(p,γ)~7Be cross section revealed a possible resonance-like structure at center of mass energy of 195 keV. The observed S-factor could be reproduced introducing a new ~7Be excited state with E ≈ 5800 keV and J~π = (1/2~+, 3/2~+). If confirmed, such excited state might also correspond to a resonance in the ~3He(~4He,γ)~7Be reaction. A new measurement of the ~6Li(p,γ)~7Be cross section at proton energies between 80 and 400 keV has been performed at the Laboratory for Underground Nuclear Astrophysics. A description of the experimental setup and preliminary results of the data analysis is provided.
机译:〜6Li(p,γ)〜7be反应涉及许多天体物理场景,从大爆炸核酸合成到主要序列恒星演化和太阳中子菌。在天体物理能量上,质子捕获〜6LI通过〜6LI(p,α)〜3he和〜6li(p,γ)〜7be反应进行。近6LI(P,γ)〜7BE横截面的近期测量揭示了在195keV的质量能量中心的可能共振结构。观察到的S因子可以再现在具有E≈5800kev和j〜π=(1/2〜+,3/2〜+)的新〜7be激发态。如果确认,这种激发状态也可能对应于〜3He(〜4He,γ)〜7BE反应中的共振。在地下核天体物理学的实验室已经进行了80至400keV的质子能量的〜6Li(P,γ)〜7BE横截面的新测量。提供了对数据分析的实验设置和初步结果的描述。

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