首页> 外文会议>International Workshop on Neutrino-Nucleus Interactions in the Few GeV Region >RCNP E398 ~(16)O,~(12)C(p,p') Experiment: Measurement of The y-ray Emission Probability from Giant Resonances in Relation To ~(16)O,~(12)C(v,v') Reactions
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RCNP E398 ~(16)O,~(12)C(p,p') Experiment: Measurement of The y-ray Emission Probability from Giant Resonances in Relation To ~(16)O,~(12)C(v,v') Reactions

机译:RCNP E398〜(16)o,〜(12)c(p,p')实验:测量与〜(16)o,〜(12)c(v,v ')反应

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We propose to measure the y-ray emission probability from excited states above 5 MeV including giant resonance of ~(16)0 and ~(12)C as a function of excitation energy in 1-MeV step. Here, we measure both the excitation energy (E_x=5-30MeV) at the forward scattering angles (0°-3°) of the ~(16)O, ~(12)C (p, p') reaction using Grand-Raiden Spectrometer and the energy of γ-rays (E_γ) using an array of NaI(Tl) counters. The purpose of the experiment is to provide the basic and important information not only for the y-ray production from primary neutral-current neutrino-oxygen (-carbon) interactions but also for that from the secondary hadronic (neutron-oxygen and -carbon) interactions.
机译:我们建议测量从5MeV以上的激发态的Y射线发射概率,包括〜(16)0和〜(12)C的巨型共振,作为1-MeV步骤中的激发能量的函数。在这里,我们使用Grand-(16)O,〜(12)C(P,P')反应的前向散射角(0°-3°)的激发能量(E_X = 5-30mev)测量使用NaI(TL)计数器阵列的γ光谱仪和γ射线(E_γ)的能量。实验的目的是提供来自初级中性中性中性 - 氧( - Carbon)相互作用的Y射线产生的基本和重要信息,而且还为来自次级Rehronic(中子氧和 - 碳)的Y射线产生互动。

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