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Energy dependent production and radionuclidic purity of [Formula: see text]from [Formula: see text]reactions: a combined theoretical and data from EXFOR library using the EMPIRE code.

Created on 27 Jun 2026

Authors

Hailu Geremew Zeleke

Published in

EJNMMI radiopharmacy and chemistry. Jun 27, 2026. Epub Jun 27, 2026.

Abstract

The production of Scandium-47, a promising radionuclide for targeted radionuclide therapy, was investigated via proton-induced reactions on enriched Ca-48 using the EMPIRE nuclear reaction code. A comparative analysis between EMPIRE simulations and experimental data extracted from EXFOR was performed for Sc-48, Sc-47, and Sc-46 production channels, showing good overall agreement, as indicated by low MAPE values and correlation coefficients close to unity. Excitation functions for the ⁴⁸Ca(p, n)⁴⁸Sc, ⁴⁸Ca(p,2n)⁴⁷Sc, and ⁴⁸Ca(p,3n)⁴⁶Sc reactions were calculated over a wide proton energy range, and thick-target yields were evaluated using stopping power data. The RNP of ⁴⁷Sc was determined as a function of incident proton energy.
The results show that radionuclide production strongly depends on proton energy. At low energies (0-12 MeV), the ⁴⁸Ca(p, n) reaction dominates, leading to significant ⁴⁸Sc formation and low RNP (~ 9%). In the intermediate energy range (12-28 MeV), the yield of ⁴⁷Sc increases substantially while maintaining relatively high purity. A more detailed analysis identifies the 16.5-21.5 MeV window as optimal, providing high yield with an RNP of approximately 94%. At higher energies (28-50 MeV), the increasing contribution of the ⁴⁸Ca(p,3n) reaction results in significant formation of long-lived ⁴⁶Sc, reducing radionuclidic purity.
These findings demonstrate that careful selection of the proton energy window is essential for optimizing both production yield and RNP, providing practical guidance for cyclotron-based production of ⁴⁷Sc for medical applications.

PMID:
42364070
Bibliographic data and abstract were imported from PubMed on 27 Jun 2026.

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