17–21 Jul 2023
MAISON MINATEC
Europe/Paris timezone

Cross sections for 54Fe(n,n') 54Fe and 54Fe(n,p') 54Mn deduced from the detection of de-excitation  rays

18 Jul 2023, 17:10
15m
Oral Nuclear Reactions Session 7B

Speaker

Sally Hicks (University of Kentucky; University of Dallas)

Description

Iron is an important component of many structural materials; examples include energy production complexes, laboratories, devices, and shipping containers that often cross borders. The properties of iron alloys in the structural materials—strength, ductility, and stability—depend on defects that develop and grow from neutron scattering and (n, p) and (n, ) reaction rates. 54Fe is only 5.5% abundant, but neutron scattering cross sections and reaction rates for this nucleus can affect fast reactor systems and energy transport and deposition. Neutron scattering cross sections obtained by the detection of the scattered neutrons offers the clearest path to the desired cross sections in the fast neutron region1, but such measurements are typically limited to scattering from only the lowest few excited levels because of the large energy spreads (10s to 100s of keV) inherent in neutron experiments. The detection of de-excitation  rays (< 2.5 keV resolution) following inelastic scattering or proton production on 54Fe offers a rare opportunity to investigate (n, p) and (n, n') cross sections to higher-lying levels in a consistent way by the examination of -ray production rates.
Measurements have been performed on an enriched 54Fe sample (97.6%) using the neutron production and -ray detection facilities at the University of Kentucky Accelerator Laboratory. -ray excitation functions were measured for incident neutron energies from 1.5 to 4.7 MeV. Angular distributions and Doppler shifts were measured at En = 4.5 MeV. -ray production cross sections were deduced by considering all  rays feeding or resulting from the decay of each level. Analogous measurements were made on natural Ti, V, Al and Fe samples for absolute normalization purposes. The results of our measurements will be presented in comparison to evaluated data (ENDF, JENDL, JEFF libraries) and with TALYS calculations.
This work was supported by the U.S. Department of Energy NNSA-SSAP award NA-0002931 and Nuclear Energy Universities Program award NU-12-KY-UK-0201-05, the U.S. National Science Foundation under grant PHY-1305801, and the U.S. National Isotope Development Program.

[1] J. R. Vanhoy et al., Nucl. Phys. A 972, 107 (2018).

Primary authors

Sally Hicks (University of Kentucky; University of Dallas) R. L. Pecha (University of Dallas) Thaddeus Howard (University of Dallas) A. J. French (University of Dallas) Z. C. Santonil (University of Dallas) J. R. Vanhoy (United States Naval Academy) A. P. D. Ramirez (University of Kentucky) E. E. Peters (University of Kentucky) S. H. Liu (University of Kentucky) F. M. Prados-Estévez (University of Kentucky) T. J. Ross (University of Kentucky) B. P. Crider (Mississippi State University) S. W. Yates (University of Kentucky)

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