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首页> 外文期刊>Physical Review C:Nuclear Physics >Stellar (n,γ) cross sections of p-process isotopes Part I: 102Pd, 120Te, 130,132Ba, and 156Dy
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Stellar (n,γ) cross sections of p-process isotopes Part I: 102Pd, 120Te, 130,132Ba, and 156Dy

机译:p-过程同位素的恒星(n,γ)截面第I部分:102Pd,120Te,130,132Ba和156Dy

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We have investigated the (n,γ) cross sections of p-process isotopes with the activation technique. The measurements were carried out at the Karlsruhe Van de Graaff accelerator using the 7Li(p,n)7Be source for simulating a Maxwellian neutron distribution of kT=25 keV. Stellar cross section measurements are reported for the light p-process isotopes 102Pd, 120Te, 130,132Ba, and 156Dy. In a following paper the cross sections of 168Yb, 180W, 184Os, 190Pt, and 196Hg will be discussed. The data are extrapolated to p-process energies by including information from evaluated nuclear data libraries. The results are compared to standard Hauser-Feshbach models frequently used in astrophysics.
机译:我们已经用活化技术研究了p-过程同位素的(n,γ)截面。使用7Li(p,n)7Be源在Karlsruhe Van de Graaff加速器上进行测量,以模拟kT = 25 keV的麦克斯韦中子分布。报道了轻质p-过程同位素102Pd,120Te,130,132Ba和156Dy的恒星横截面测量。在以下论文中,将讨论168Yb,180W,184Os,190Pt和196Hg的横截面。通过包括来自评估核数据库的信息,可将数据外推至p过程能。将结果与天体物理学中常用的标准Hauser-Feshbach模型进行比较。

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