Determination of the 233Pa(n, γ) capture cross section up to neutron energies of 1 MeV using the transfer reaction 232Th(3He, p)234Pa∗
Autor: | D. Dassié, L. Perrot, E. Berthoumieux, F. Gunsing, S. Czajkowski, S. Boyer, Ch. Theisen, M. Aiche, C. Grosjean, G. Aerts, B. Haas, A. Guiral, J. N. Wilson, N. Thiollière, G. Barreau, B. Osmanov |
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Rok vydání: | 2006 |
Předmět: |
Nuclear reaction
Physics Nuclear and High Energy Physics Range (particle radiation) 010308 nuclear & particles physics Astrophysics::High Energy Astrophysical Phenomena Inelastic scattering Scintillator 01 natural sciences 7. Clean energy Neutron temperature Charged particle Cross section (physics) 0103 physical sciences Neutron Atomic physics 010306 general physics |
Zdroj: | Nuclear Physics A. 775:175-187 |
ISSN: | 0375-9474 |
DOI: | 10.1016/j.nuclphysa.2006.06.013 |
Popis: | The γ -ray emission probability distribution of 234 Pa ∗ has been measured between 5.2 and 6.2 MeV excitation energy using the transfer reaction 232 Th( 3 He, p) 234 Pa ∗ at an incident 3 He energy of 24 MeV. The experimental set-up is made of four liquid scintillator C 6 D 6 detectors and four Si telescopes arranged to detect γ rays and charged particles in coincidence. In order to determine the total number of γ -ray cascades in a given nucleus, the raw experimental detected gamma-ray events have to be corrected by the weighting function technique. This weighting requires complete knowledge of the efficiency and response functions for the C 6 D 6 detector set-up and surroundings. These have been determined experimentally using gamma-ray sources, inelastic scattering reactions and transfer reactions on light nuclei. Simulations which reproduce successfully the detector response and efficiency are presented. From these measurements, the (n, γ ) capture cross section of 233 Pa, in the neutron energy range 0 to 1 MeV, has been deduced via the product of the measured γ emission probability of 234 Pa ∗ with the calculated compound nucleus formation cross section of the reaction 233 Pa + n. A comparison between existing data bases or recent predictions and the present results is also made. |
Databáze: | OpenAIRE |
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