Energy release in Be, C and W due to irradiation with D and T atoms

D. Meluzova, P. Babenko, M. Mironov, V. S. Mikhailov, A. Shergin, A. Zinoviev
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Abstract

The distribution of the energy release over the depth of the material was calculated for hydrogen isotopes bombarding beryllium, carbon and tungsten surfaces. It was shown that for energies less than 50 keV the maximum energy release occurs near the surface. The distribution of the energy release over depth was calculated for the energy spectra of neutral particles typical for the ITER tokamak-reactor. Obtained data makes it possible to estimate the heating of the near-surface layers when the walls are bombarded by atoms leaving the plasma. The accumulation of tritium in the surface layers is predicted.The distribution of the energy release over the depth of the material was calculated for hydrogen isotopes bombarding beryllium, carbon and tungsten surfaces. It was shown that for energies less than 50 keV the maximum energy release occurs near the surface. The distribution of the energy release over depth was calculated for the energy spectra of neutral particles typical for the ITER tokamak-reactor. Obtained data makes it possible to estimate the heating of the near-surface layers when the walls are bombarded by atoms leaving the plasma. The accumulation of tritium in the surface layers is predicted.
由于D和T原子辐照,Be、C和W中的能量释放
计算了氢同位素轰击铍、碳和钨表面的能量释放在材料深度上的分布。结果表明,当能量小于50kev时,最大能量释放发生在表面附近。计算了ITER托卡马克反应堆典型中性粒子能谱在深度上的能量释放分布。获得的数据使我们能够估计出当等离子体的原子轰击壁面时,近表层的加热情况。预测了氚在表层的积累。计算了氢同位素轰击铍、碳和钨表面的能量释放在材料深度上的分布。结果表明,当能量小于50kev时,最大能量释放发生在表面附近。计算了ITER托卡马克反应堆典型中性粒子能谱在深度上的能量释放分布。获得的数据使我们能够估计出当等离子体的原子轰击壁面时,近表层的加热情况。预测了氚在表层的积累。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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