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2025 ANS Winter Conference & Expo
November 8–12, 2025
Washington, DC|Washington Hilton
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Nuclear News 40 Under 40—2025
Last year, we proudly launched the inaugural Nuclear News 40 Under 40 list to shine a spotlight on the exceptional young professionals driving the nuclear sector forward as the nuclear community faces a dramatic generational shift. We weren’t sure how a second list would go over, but once again, our members resoundingly answered the call, confirming what we already knew: The nuclear community is bursting with vision, talent, and extraordinary dedication.
Liu Xiaobo, Fan Xiaoqiang, Peng Xianjue, Du Jinfeng, Gao Hui
Nuclear Science and Engineering | Volume 179 | Number 2 | February 2015 | Pages 119-129
Technical Paper | doi.org/10.13182/NSE13-30
Articles are hosted by Taylor and Francis Online.
A novel experimental method is introduced for effectively validating neutron initiation probability, through which the delayed neutron influence on the source strength can be neglected—this is the main reason for substantially explaining the burst waiting time experiments performed in the Godiva and Caliban burst reactors. The key idea of the new method is that the burst is initiated by simultaneously injecting a pulse of neutrons with appropriate strength just as the reactor achieves prompt supercritical and tallied by judging whether or not the burst is initiated by the pulsed neutrons based on the measured data. The principle of the method is described using initiation theory. The Chinese Fast Burst Reactor–II (CFBR-II) structure and two sets of configurations for preliminary experiments are then described. Last, those two sets of preliminary experiments are carried out on CFBR-II in the state of 0.042 $ prompt supercritical, and results, including the typical picture and other important measured data, are provided in order to illustrate how the initiation probability can be validated. The initiation probability of 0.43 was determined by preliminary performing of 65 bursts, which is an ∼35% relative difference between the theoretic calculations and the experimental results. Some discussion and suggestions for possible follow-on work are provided.