Study of secondary neutron interactions with 232Th, 129I, and 127I nuclei with the uranium assembly “QUINTA” at 2, 4, and 8GeV deuteron beams of the JINR Nuclotron accelerator

The natural uranium assembly, “QUINTA”, was irradiated with 2, 4, and 8GeV deuterons. The 232Th, 127I, and 129I samples have been exposed to secondary neutrons produced in the assembly at a 20-cm radial distance from the deuteron beam axis. The spectra of gamma rays emitted by the activated 232Th, 1...

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Published inApplied radiation and isotopes Vol. 107; no. C; pp. 225 - 233
Main Authors Adam, J., Chilap, V.V., Furman, V.I., Kadykov, M.G., Khushvaktov, J., Pronskikh, V.S., Solnyshkin, A.A., Stegailov, V.I., Suchopar, M., Tsoupko-Sitnikov, V.M., Tyutyunnikov, S.I., Vrzalova, J., Wagner, V., Zavorka, L.
Format Journal Article
LanguageEnglish
Published United States Elsevier Ltd 01.01.2016
Elsevier
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Summary:The natural uranium assembly, “QUINTA”, was irradiated with 2, 4, and 8GeV deuterons. The 232Th, 127I, and 129I samples have been exposed to secondary neutrons produced in the assembly at a 20-cm radial distance from the deuteron beam axis. The spectra of gamma rays emitted by the activated 232Th, 127I, and 129I samples have been analyzed and several tens of product nuclei have been identified. For each of those products, neutron-induced reaction rates have been determined. The transmutation power for the 129I samples is estimated. Experimental results were compared to those calculated with well-known stochastic and deterministic codes. •The natural uranium assembly, "QUINTA", was irradiated with 2, 4, and 8GeV deuterons. The 232Th, 127I, and 129I samples have been exposed to secondary neutrons produced in the assembly at a 20-cm radial distance from the deuteron beam axis.•The spectra of gamma rays emitted by the activated 232Th, 127I, and 129I samples have been analyzed and several tens of product nuclei have been identified.•For each of those products, neutron-induced reaction rates have been determined.•The transmutation power for the 129I samples is estimated.•Experimental results were compared to those calculated with well-known stochastic and deterministic codes.
Bibliography:AC02-07CH11359
USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
FERMILAB-PUB-16-215-APC
ISSN:0969-8043
1872-9800
DOI:10.1016/j.apradiso.2015.11.002