Elmaghraby E K, Said S A, Asfour F I
Experimental Nuclear Physics Department, Nuclear Research Center, Atomic Energy Authority, Cairo 13759, Egypt.
Appl Radiat Isot. 2009 Jan;67(1):147-51. doi: 10.1016/j.apradiso.2008.07.017. Epub 2008 Jul 31.
Radioactive isotopes of antimony could be produced from proton induced reactions on tin isotopes. At low energy, (p,n) reactions are the only open channels. Measurements are performed for proton reactions with (124)Sn in the energy range between 9.0 and 18.0MeV. Evaluations of the remaining possible reactions are performed and compared with each other. The cross sections are calculated theoretically by the EMPIRE-II code for (124)Sn(p,n)(124)Sb reaction. However, the calculations failed to agree with the experimental results. A recommended evaluation is given and the thick target yields are calculated from the evaluated approximations.
锑的放射性同位素可通过质子与锡同位素的反应产生。在低能量下，(p,n)反应是唯一开放的通道。对能量范围在9.0至18.0 MeV之间的质子与(124)Sn的反应进行了测量。对其余可能的反应进行了评估并相互比较。通过EMPIRE-II代码对(124)Sn(p,n)(124)Sb反应的截面进行了理论计算。然而，计算结果与实验结果不一致。给出了推荐的评估，并根据评估的近似值计算了厚靶产额。
