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Investigating ~(13)C+~(12)C Reaction by the Activation Method. Sensitivity Tests

机译:采用活化法研究〜(13)C +〜(12)C反应。敏感性测试

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We have performed experiments to check the limits of sensitivity of the activation method using the new 3 MV Tandetron accelerator and the low and ultra-low background laboratories of the "Horia Hulubei" National Institute of Physics and Nuclear Engineering (IFIN-HH). We have used the ~(12)C+~(13)C reaction at beam energies E_(lab)= 6, 7 and 8 MeV. The knowledge of this fusion cross section at deep sub-barrier energies is of interest for astrophysical applications, as it provides an upper limit for the fusion cross section of ~(12)C+~(12)C over a wide energy range. A ~(13)C beam with intensities 0.5- 2 particleμA was provided by the accelerator and used to bombard graphite targets, resulting in activation with ~(24)Na from the ~(12)C(~(13)C,p) reaction. The 1369 and 2754 keV gamma-rays from ~(24)Na de-activation were clearly observed in the spectra obtained in two different laboratories used for measurements at low and ultralow background: one at the surface and one located underground in the Unirea salt mine from Slanic Prahova, Romania. In the underground laboratory, for E_(lab)= 6 MeV we have measured an activity of 0.085 ± 0.011 Bq, corresponding to cross sections of 1-3 nb. This demonstrates that it is possible to measure ~(12)C targets irradiated at lower energies for at least 10 times lower cross sections than before. β-γ coincidences will lead us another factor of 10 lower, proving that this installations can be successfully used for nuclear astrophysics measurements.
机译:我们已经进行了实验,以检查激活方法的灵敏度限制,使用新的3 MV Tandetron加速器和“Horia Hulubei”国家物理和核工程研究所(Ifin-HH)的低和超低背景实验室。我们使用了〜(12)C +〜(13)C在Chap Energies E_(实验室)= 6,7和8 MeV处的反应。对于天体物理应用,这种融合横截面的知识对天体物理应用感兴趣,因为它为宽能量范围内的〜(12)C +〜(12)C的融合横截面提供了上限。促进剂提供〜(13)C光束0.5-2颗粒μA,并用来轰击石墨靶,从〜(12)c(〜(13)c,p)中,用〜(24)Na活化反应。来自〜(24)Na去活化的1369和2754 kevγ射线在用于在低和超级背景下测量的两种不同实验室中获得的光谱中清楚地观察到〜(24)的光谱中:一个在地表和一个位于Unirea盐矿地下的地下来自罗马尼亚的Slanic Prahova。在地下实验室,对于E_(实验室)= 6 MEV,我们已经测量了0.085±0.011 BQ的活动,对应于1-3 NB的横截面。这表明可以测量在较低能量下照射的〜(12)C目标比以前的横截面较低的10倍。 β-γ巧合将导致我们的另一个因素为10,证明该装置可以成功用于核天体物理测量。

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