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Excitation functions of the reactions nat Sb(α,xn) 123,124,125,126 I, 121 Sb(α,xn) 123,124 I, nat Sb( 3 He,xn) 121,123,124 and 126 Te(p,xn) 123,124,125,126 I were measured from the respective threshold up to 22 MeV α-, 36 MeV 3 He- and 100 MeV p-energy, with particular emphasis on data for the production of the medically important radionuclide 124 I. The conventional stacked-foil technique was used. The optimum energy range and yield for the production of 124 I were determined. The isotopic impurities in the produced 124 I are discussed. A comparison of all production routes of 124 I is given, including other (p,xn) and (d,xn) nuclear reactions already known. The α -a nd 3 He-induced reactions on antimony are not suitable for the production of 124 I due to low batch yield and high impurity level. The commonly used production route 124 Te(p,n) 124 I gives the purest form of 124 I and the production can be done at a small-sized cyclotron. Large scale production via 125 Te(p,2n) or 126 Te(p,3n) reaction is possible, but with a higher impurity level. Cyclotrons with higher proton energy are needed (up to 40 MeV). The final choice will depend upon the tolerable level of impurities.

Comparative studies on the production of the medically important radionuclide <sup>124</sup>I via p-, d-, <sup>3</sup>He- and α-particle induced reactions

Comparative studies on the production of the medically important radionuclide 124I via p-, d-, 3He- and α-particle induced reactions

Comparative studies on the production of the medically important radionuclide ¹²⁴I via p-, d-, ³He- and α-particle induced reactions