作者: A. Nikjou , M. Sadeghi
DOI: 10.1016/J.APRADISO.2018.02.003
关键词:
摘要: Abstract The 123I radionuclide (T1/2 = 13.22 h, β+ = 100%) is one of the most potent gamma emitters for nuclear medicine. In this study, cyclotron production via different reactions namely, 121Sb(α,2n), 122Te(d,n), 123Te(p,n), 124Te(p,2n), 124Xe(p,2n), 127I(p,5n) and 127I(d,6n) were investigated. effect various phenomenological level density models such as Fermi gas model (FGM), Back-shifted (BSFGM), Generalized superfluid (GSM) Enhanced generalized (EGSM) moreover, three microscopic evaluated predicting cross sections yield predictions. SRIM code was used to obtain target thickness. excitation function calculated by using TALYS-1.8, EMPIRE-3.2 codes with data which taken from TENDL-2015 database, finally theoretical calculations compared reported experimental measurements in EXFOR database.