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Astrophysical S-factor for the radiative capture reaction 13C(p,g)14N

机译:用于辐射捕获反应的天体物理s因子13C(p,g)14N

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摘要

The phase shift analysis, done on the basis of the known measurements of thedifferential cross-sections of the p13C elastic scattering at the energy range250-750 keV, shows that it is enough to take into account only 3S1 wave in theconsidered energy region. The potential for the triplet 3S1 state in p13Csystem at the resonance energy 0.55 MeV corresponding to quantum numbers JpT =1-1 as well as the potential for the 3P1 bound state of 14N were constructed onthe basis of the obtained scattering phase shifts. The possibility to describethe experimental data of the astrophysical S-factor of the p13C radiativecapture at the energies 0.03-0.8 MeV was considered within the potentialcluster model with the forbidden states. It was shown that we properly succeedin explanation of the energy behavior of the astrophysical S-factor for thep13C radiative capture at the resonance energy range 0.55 MeV (laboratorysystem).
机译:在能量范围为250-750 keV的p13C弹性散射的微分截面的已知测量的基础上进行的相移分析表明,仅考虑考虑的能量区域中的3S1波就足够了。基于获得的散射相移,构造了p13C系统中三重态3S1态的电势,共振能量为0.55 MeV,对应于量子数JpT = 1-1,以及3P1键态的14N。在具有禁止状态的势能簇模型中,考虑了在能量为0.03-0.8 MeV时描述p13C辐射捕获天体S因子实验数据的可能性。结果表明,我们正确地解释了在共振能范围0.55 MeV(实验室系统)下p13C辐射捕获的天体S因子的能量行为。

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