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North American construction is back—smaller and faster—at OPG’s Darlington
“The nuclear renaissance is real here,” said Ontario Power Generation’s Subo Sinnathamby on May 8, one year to the day after OPG secured a final investment decision to build the first of four planned BWRX-300 reactors at its Darlington nuclear power plant, and shortly after the new reactor’s foundation was lifted into place. “We got our license to construct in April and our [final investment decision] in May, and we’ve been off to the races since.”
Yong-Qian Shi, Pu Xia, Zhang-Lin Luo, Zhi-Xiang Zhao, Dazhao Ding, Yi-Guo Li, Qin-Fu Zhu, Hai-Hong Xia, Ji-Gen Li, Wei Zhang, Jian Cao, Yan-Hui Quan, Huang-Da Luo, Xiaofei Wu
Nuclear Technology | Volume 159 | Number 1 | July 2007 | Pages 106-118
Technical Paper | Accelerators | doi.org/10.13182/NT07-A3858
Articles are hosted by Taylor and Francis Online.
The paper presents the design objectives and structure of China's accelerator-driven subcritical system subcritical assembly Venus-1. The core of Venus-1 is a coupled core with a fast neutron zone and a thermal neutron zone. The fast neutron zone is at the center of the core and is formed by natural uranium fuel. A fast neutron spectrum field can be produced in the fast neutron zone and used for transmutation. The thermal neutron zone surrounds the fast neutron zone and is formed by low-enriched uranium fuel; it is a fission zone. Venus-1 is driven by an Am-Be or other steady neutron source (252Cf, D-D reaction or D-T reaction) to research the effect of an external neutron source with different energies on it or is driven by a D-T pulsed neutron source through the China Institute of Atomic Energy pulsed neutron generator to research the dynamic characteristic. On July 18, 2005, the first fuel element was loaded into the Venus-1 subcritical assembly, and some preliminary experiments on subcritical and neutron distribution have been performed. The final load has been determined by preliminary experiments on Venus-1. The relative neutron importance of the external source, the relative distribution of the thermal neutron flux in the fast neutron zone, and the variation of the neutron count with the addition of natural uranium fuel also have been determined by preliminary experiments on Venus-1.