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OSTP memo guides space nuclear plan
A White House Office of Science and Technology Policy (OSTP) memorandum released on Tuesday guides NASA, the Department of Energy, and the Department of Defense on their roles in deploying near-term space nuclear power.
This follows a series of NASA announcements last month—driven by the executive order “Ensuring American Space Superiority,” issued by Trump in December—including an ambitious timeline for establishing a moon base, which would rely on fission surface power (FSP) to survive the long lunar night at the moon’s south pole, and plans for a nuclear electric propulsion (NEP) rocket to be launched in 2028.
Shen Zhang, Nan Gui, Xingtuan Yang
Nuclear Science and Engineering | Volume 199 | Number 7 | July 2025 | Pages 1073-1090
Research Article | doi.org/10.1080/00295639.2024.2437937
Articles are hosted by Taylor and Francis Online.
Nuclear reactions generate large temperature differences in materials, causing change in the density of the materials. An uneven density distribution means the macroscopic cross section will change in spatial locations, even within the same material. This scenario makes the neutron transport calculation difficult. However, this issue can be solved by developing an algorithm for neutron transport in volume meshes that stores data about how the medium density changes with space and tracks the neutron in barycentric coordinates.
This study proposes such a novel method by incorporating the barycentric particle tracking algorithm into Monte Carlo transport within volume meshes. The method involves the introduction of face search algorithms, particle-face distance calculation algorithms, and the resolution of compatibility between the distance algorithm and the tracking algorithm. Consequently, the computational results and evaluations performed by our code and the OpenMC code across diverse geometric configurations and enrichments exhibit a noteworthy degree of consistency. The discrepancies in the simulation results between the two codes are all within ±3σ. Therefore, the algorithm’s correctness is affirmed. Moreover, the computational time of the current method displays a logarithmic function–like relationship with the number of meshes, which means the computational performance is highly efficient and desirable.
Finally, the application of the current model in some irregular geometries and geometries with varied temperature distributions is demonstrated. The results prove that the Monte Carlo particle transport method can also be directly applied to these situations. All of this illustrates the future ability of the current method to calculate neutron transport in reactors of extremely nonuniformly distributed physical fields and irregular geometry at relatively tiny geometric scales.