2017
DOI: 10.1088/2053-1591/aa8c22
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Helium, hydrogen, and fuzz in plasma-facing materials

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Cited by 122 publications
(78 citation statements)
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“…An evolution of porous structure to coral-like structure is observed. Coral-like structure (a mixture of fuzzy structure and deep holes [20]) on polycrystalline W after with similar high heat flux He neutral beams injection is widely reported, even at a higher surface temperature up to 2700 °C [11,18,19]. Coral-like structures on W-enriched region are uniformly distributed.…”
Section: Surface Modification After He Loading At a High Peak Surfacementioning
confidence: 87%
See 1 more Smart Citation
“…An evolution of porous structure to coral-like structure is observed. Coral-like structure (a mixture of fuzzy structure and deep holes [20]) on polycrystalline W after with similar high heat flux He neutral beams injection is widely reported, even at a higher surface temperature up to 2700 °C [11,18,19]. Coral-like structures on W-enriched region are uniformly distributed.…”
Section: Surface Modification After He Loading At a High Peak Surfacementioning
confidence: 87%
“…Blistering and lids exfoliation are shown on the surface of W-5V after exposed to repeated He pulses at a low peak surface temperature of 900 °C, while porous structure and coral-structure are dominant at a high peak surface temperature of 1800 °C. He bubble growth and rupture are the main factors of He-induced surface modification [20,21]. The effect of surface temperature and He fluence on He bubble evolution and surface modification is discussed.…”
Section: Discussionmentioning
confidence: 99%
“…Helium bubble growth in plasma-facing materials (PFMs) is an important aspect of nuclear fusion materials research [1][2][3] . Not only do helium bubbles cause material embrittlement and fatigue, but helium also causes significant damage to plasma-facing surfaces in the form of fuzz or coral-like features [4][5][6][7] , and modelling these phenomena continues to be a challenge [8][9][10][11] .…”
mentioning
confidence: 99%
“…Besides bubbles, blistering can be formed, when the highly pressurized fine bubbles, formed close to the projected range of the incident ions, mediate inter bubble cracking [118]. At higher temperatures (1073-1273 K), when vacancies and helium bubbles can migrate thermally, large helium bubbles form [118,120]. With increase in helium fluence and temperature, bubbles can evolve into 'nanofuzz' structures (generally forming between 1000 and 2000 K) as shown in Fig.…”
Section: The Effect Of Helium On the Plasma-facing Componentmentioning
confidence: 99%