Atomization and Transport of Radionuclides in Plasma for Ion-Plasma Deactivation Technology for NPP Equipment and SNF Processing

IF 0.4 4区 物理与天体物理 Q4 PHYSICS, NUCLEAR Physics of Atomic Nuclei Pub Date : 2025-02-19 DOI:10.1134/S1063778824090266
A. S. Petrovskaya, A. B. Tsyganov
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Abstract

This paper is devoted to the actual problems of nuclear energy: deactivation of nuclear power plants (NPPs), hot cells, equipment for isotope separation, and reprocessing of spent nuclear fuel (SNF) to effectively close the nuclear fuel cycle. The authors have proposed the ion-plasma “dry” technology developed to solve these problems. The operating parameters of the ion-plasma technology for deactivation and reprocessing of spent nuclear fuel have been obtained: inert gas pressure of 0.1–1 atm., inert carrier gas flow rate of 1–10 m/s, and current density of 1–5 A/cm2 at the operating voltage of 100–1000 V. Using the example of SNF processing, the ranges of partial pressures and deposition temperatures of SNF elements during the process of its separation according to elemental composition have been calculated. Because of the difference in the condensation temperature ranges of each spent fuel element, purification of uranium and plutonium from most fission products of MOX and MNUP spent fuel with a purity of at least 99% has been demonstrated.

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核电站设备离子等离子体失活技术及SNF处理中放射性核素在等离子体中的原子化和输运
本文致力于核能的实际问题:核电厂(NPPs)的停用,热电池,同位素分离设备,以及乏核燃料(SNF)的后处理,以有效地关闭核燃料循环。为了解决这些问题,作者提出了离子等离子体“干”技术。获得了离子等离子体技术用于乏燃料失活后处理的操作参数:惰性气体压力为0.1 - 1atm。惰性载气流速为1 ~ 10m /s,工作电压为100 ~ 1000v,电流密度为1 ~ 5a /cm2。以SNF加工为例,根据元素组成计算了SNF分离过程中各元素的分压和沉积温度范围。由于每个乏燃料元件的冷凝温度范围不同,从MOX和MNUP乏燃料的大多数裂变产物中纯化铀和钚的纯度至少达到99%。
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来源期刊
Physics of Atomic Nuclei
Physics of Atomic Nuclei 物理-物理:核物理
CiteScore
0.60
自引率
25.00%
发文量
56
审稿时长
3-6 weeks
期刊介绍: Physics of Atomic Nuclei is a journal that covers experimental and theoretical studies of nuclear physics: nuclear structure, spectra, and properties; radiation, fission, and nuclear reactions induced by photons, leptons, hadrons, and nuclei; fundamental interactions and symmetries; hadrons (with light, strange, charm, and bottom quarks); particle collisions at high and superhigh energies; gauge and unified quantum field theories, quark models, supersymmetry and supergravity, astrophysics and cosmology.
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