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Front-end nuclear fuel supply cooperation: Turning allied interdependence into strategic advantage
The global nuclear revival, which is fueled by unprecedented demand for firm, affordable, dispatchable power for artificial intelligence and data center build-out, energy security imperatives, and climate commitments, has exposed a structural reality of the Western fuel cycle: No single allied nation currently possesses the full suite of front-end capabilities. From mining through conversion, enrichment, fabrication, and the emerging deconversion and metallization steps required for reactor fuels, capability is distributed across Canada, France, Japan, the United Kingdom, and the United States (collectively, the “Sapporo Five”), as well as a small group of close partners.
K. Wisshak, F. Käppeler, G. Reffo
Nuclear Science and Engineering | Volume 88 | Number 4 | December 1984 | Pages 594-598
Technical Note | doi.org/10.13182/NSE84-A18376
Articles are hosted by Taylor and Francis Online.
The neutron capture width of the s-wave resonance at 34.8 keV in 27Al has been determined using a setup with extremely low neutron sensitivity. This feature is important because this resonance exhibits a very large scattering-to-capture ratio. A pulsed 3-MV Van de Graaff accelerator and a kinematically collimated neutron beam, produced via the 7Li(p,n) reaction, were used in the experiment. Capture gamma rays were observed by three Moxon-Rae detectors with graphite, bismuth-graphite, and bismuth converters, respectively. The samples were positioned at a neutron flight path of only 9 cm. Thus, events due to capture of resonance-scattered neutrons in the detectors or in surrounding materials are completely discriminated by their additional time of flight. The data obtained with the individual detectors were corrected for the efficiency of the different converter materials. For that purpose, theoretical calculations of the capture gamma-ray spectra of the measured isotope and of gold, which was used as a standard, were performed. The final radiative width is gΓγ = 1.22 ± 0.07 eV. The accuracy is a factor of ∼3 better than in previous experiments.