2000
DOI: 10.1016/s0022-3115(00)00289-0
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Microstructure evolution in tungsten during low-energy helium ion irradiation

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Cited by 351 publications
(199 citation statements)
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“…The most stable configuration for He atoms, all of them in interstitial position, is in a platelet configuration at 0 K [66]. The high binding energies indicate that these clusters are stable at temperatures under 500 K. This is in agreement with platelets experimentally observed by Iwakiri et al [45], after irradiating W with 0.25 keV He ions at 293 K, as they observed platelets formed by He atoms. In the case of mixed He-SIA clusters (He n I m ), the binding energies proposed by Becquart et al [66] have been used, i.e., single He atoms bind to SIA (I) and SIA clusters (I n ) with a binding energy of 0.94 eV.…”
Section: Helium In Tungstensupporting
confidence: 89%
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“…The most stable configuration for He atoms, all of them in interstitial position, is in a platelet configuration at 0 K [66]. The high binding energies indicate that these clusters are stable at temperatures under 500 K. This is in agreement with platelets experimentally observed by Iwakiri et al [45], after irradiating W with 0.25 keV He ions at 293 K, as they observed platelets formed by He atoms. In the case of mixed He-SIA clusters (He n I m ), the binding energies proposed by Becquart et al [66] have been used, i.e., single He atoms bind to SIA (I) and SIA clusters (I n ) with a binding energy of 0.94 eV.…”
Section: Helium In Tungstensupporting
confidence: 89%
“…A possible solution could be the use of nanostrucutred W [43], due to its high grain boundary (GB) density. Nanostructured W is expected to present higher irradiation tolerance [44], as GBs may act as defect sinks for vacancies, SIAs and light species [45][46][47][48]. GBs, on the one hand, might increase the annihilation rate between vacancies and SIAs and, on the other hand, might trap He and H atoms, decreasing their number in the interior of the grains.…”
Section: Acknowledgementsmentioning
confidence: 99%
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“…In addition, we have to determine the plasma and device operations that affect the reflectivity. Various plasma-surface interactions contribute to the degradation of the reflectivity: deposition of impurities (metal, carbon) on the surface [1], sputtering by ions and charge exchange particles [2], and the formation of bubbles and blisters on the surface layer [3]. These interactions depend on the plasma conditions (main discharge, glow discharge cleaning and working gas), in-vessel conditions (wall and divertor materials and the wall temperature), and mirror location.…”
Section: Introductionmentioning
confidence: 99%
“…[9], in a linear divertor plasma simulator device, it should be noted that bombarding helium atoms could create bubbles on the surface of tungsten even if their energy (< 50 eV) was much below the sputtering threshold energy (~ 0.4 keV). It was also found that the bubbles could be formed even at high temperature (~ 1,000 K) [10]. The fact that helium bubbles are remarkably formed at high temperature in tungsten even if the energy of the helium is less than or near the threshold energy for displacement damage suggests the enhancement of hydrogen trapping and difficulty controlling the recycling process for the hydrogen isotope during the burning plasma discharge.…”
Section: Introductionmentioning
confidence: 99%