利用 Serpent2 进行恒星器中子参数化建模的原理验证

Tommi Tapani Lyytinen, Antti Snicker, Joonas Virtanen, Iole Palermo, Javier Alguacil, Timo Jos Bogaarts, Felix Warmer
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引用次数: 1

摘要

本文介绍了利用 Serpent2 代码对 5 周期 HELIAS 恒星器进行的中子输运研究。这些研究利用参数化几何模型,通过改变反应堆层的厚度来实现中子建模的扫描。例如,氚孕育率(TBR)可以通过探索各种毯子材料选项和厚度来确定,从而找出符合 1.15 TBR 设计标准的阈值配置。我们发现,采用氦冷却卵石垫(HCPB)候选方案时,氚滋生区厚度为 26 厘米,即可满足氚滋生比标准;而采用双冷却锂铅(DCLL)时,厚度为 46 厘米,即可超过阈值。此外,该几何结构还包括非平面场线圈,可以研究这些超导线圈中的快中子通量,其技术极限为 1e9 1/cm2s。研究表明,线圈中的中子快通量并不是恒定的,因此有必要进行中子传输模拟,以确定线圈中的快通量分布。我们的研究表明,峰值通量可能比平均通量高出 2 倍以上,而且峰值通量的位置呈螺旋状旋转。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Proof-of-principle of parametric stellarator neutronics modeling using Serpent2
This contribution presents neutron transport studies for the 5-period HELIAS stellarator using the Serpent2 code. These studies utilize a parametric geometry model, enabling scans in neutronics modeling by varying the thickness of the reactor layers. For example, the tritium breeding ratio (TBR) can be determined by exploring various blanket material options and thicknesses to identify the threshold configuration that meets the TBR design criterion of 1.15. We found out that with the helium-cooled pebble ped (HCPB) candidate option, the TBR criterion is met with a breeding zone thickness of 26 cm, while with the dual-coolant lithium lead (DCLL) the threshold is exceeded at a thickness of 46 cm. Furthermore, the geometry includes non-planar field coils, allowing to study the fast neutron flux in these superconducting coils with a technological limit of 1e9 1/cm2s. It is shown that the neutron fast flux is not constant at the coils, necessitating a neutron transport simulation to determine the distribution of the fast-flux at the coils. We show that the peak flux can be more than a factor of 2 higher than the average flux, and that the peak flux location rotates helically.
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