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首页> 外文期刊>Journal of Nuclear Materials: Materials Aspects of Fission and Fusion >A coupled rate theory-Monte Carlo model of helium bubble evolution in plasma-facing micro-engineered tungsten
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A coupled rate theory-Monte Carlo model of helium bubble evolution in plasma-facing micro-engineered tungsten

机译:耦合速率理论蒙特卡罗模型氦泡型血浆微型微型钨中的氦气泡沫进化

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A multiscale model of helium bubble evolution in plasma-facing materials is developed. The model links different stages of helium bubble evolution: deposition, nucleation, growth, motion, and coalescence. Helium deposition is simulated with the SRIM Monte Carlo program to give spatial information on helium and displacement damage distributions near the surface. This deposition profile is then introduced into a space-dependent rate theory of bubble nucleation and growth to describe the early stages of the distribution and size of helium bubbles. The coarsening stage of bubble evolution as a result of whole bubble motion, interaction, and coalescence is modeled by a new Object Kinetic Monte Carlo (OKMC) model, for which initial conditions are taken from the mean-field rate theory calculations. The model is compared to experimental data on low-energy helium plasma interaction with micro-engineered tungsten (W), and on high-energy helium ion deposition in flat W samples. Novel features of the multiscale model include: (1) space-dependent rate theory; (2) OKMC model of bubble motion in stress and temperature fields; and (3) application of the model to micro-engineered materials, and comparison with experiments on the same time-scale. At low helium ion energy, it is found that the mechanism of trap mutation is essential in achieving good agreement with experimental measurements. On the other hand, good agreement with experiments at high incident ion energy and temperature showed the importance of bubble coalescence and coarsening as main mechanisms. The results of the model are compared with experiments on flat W surfaces irradiated at high ion energy (30 keV), and with micro-engineered W, where the surface is coated with high-density micro-pillars at low ion energy (around 100 eV). The predicted average bubble radius and density are in qualitative agreement with experimental results. Published by Elsevier B.V.
机译:开发了邻近等离子体材料中氦气泡沫进化的多尺度模型。该模型与氦气泡沫进化的不同阶段联系起来:沉积,成核,生长,运动和聚结。用Srim Monte Carlo程序模拟氦沉积,以在表面附近的氦气和位移损伤分布上提供空间信息。然后将该沉积轮廓引入泡沫成核和生长的空间依赖性速率理论中,以描述氦气泡的分布和尺寸的早期阶段。由于整个气泡运动,相互作用和聚结而产生的气泡进化的粗化阶段由新的对象动力学蒙特卡罗(OKMC)模型建模,其中初始条件是从平均场速率理论计算中取出的。该模型与微型微型钨(W)的低能量氦血浆相互作用的实验数据进行比较,以及扁平W样品中的高能氦离子沉积。多尺度模型的新功能包括:(1)空间依赖率理论; (2)OKMC压力和温度场气泡运动模型; (3)将模型应用于微型工程材料,并在同一时间尺度与实验进行比较。在低氦离子能量下,发现捕集突变机制对于实现与实验测量良好的一致性是必不可少的。另一方面,与高事故离子能量和温度的实验良好的一致性表明泡影聚结和粗化为主要机制的重要性。将模型的结果与在高离子能量(30keV)照射的扁平W表面上进行比较,并且用微型工程W,在低离子能量下用高密度微柱涂覆表面(约100eV )。预测的平均气泡半径和密度与实验结果进行定性协议。由elsevier b.v出版。

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