Production cross-section calculations of In-111 via proton and alpha-induced nuclear reactions

Ozdogan H., Sarpün İ. H., Şekerci M., Kaplan A.

MODERN PHYSICS LETTERS A, cilt.36, sa.8, 2021 (SCI-Expanded) identifier identifier

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 36 Sayı: 8
  • Basım Tarihi: 2021
  • Doi Numarası: 10.1142/s0217732321500516
  • Dergi Adı: MODERN PHYSICS LETTERS A
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus, Academic Search Premier, INSPEC, zbMATH
  • Anahtar Kelimeler: Indium, radioisotope production cross-section, TALYS 1.95, EMPIRE 3.2, EXCITATION-FUNCTIONS, HYBRID MODEL, YIELDS, DECAY
  • Akdeniz Üniversitesi Adresli: Evet

Özet

In-111, a known gamma emitter, is used for many medical purposes such as imaging of myocardial metastases. It can be produced by using different nuclear reactions. In this study, the reactions of Ag-109(alpha,2n)In-111, Cd-111(p, n)In-111, Cd-112(p, 2n)In-111, Cd-113(p, 3n)In-111 and Cd-114(p, 4n)In-111, which are the production routes of In-111, were investigated. Production cross-section calculations were performed by using equilibrium and pre-equilibrium models of TALYS 1.95 and EMPIRE 3.2 nuclear reaction codes. Hauser-Feshbach Model was appointed in both codes for calculations of equilibrium approximations. Exciton and Hybrid Monte Carlo Simulation (HMS) models were used in the EMPIRE 3.2, whereas Two-Component Exciton and Geometry Dependent Hybrid Model, which is implemented to TALYS code, has been used in the TALYS 1.95 for pre-equilibrium reactions. Also, a weighting matrix of the nuclear models was obtained by using statistical variance analysis. The optimum beam energy to obtain In-111 has been determined by using the results obtained from this weighting matrix.