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Morphologies of tungsten nanotendrils grown under helium exposure
Nanotendril “fuzz” will grow under He bombardment under tokamak-relevant conditions on tungsten plasma-facing materials in a magnetic fusion energy device. We have grown tungsten nanotendrils at low (50 eV) and high (12 keV) He bombardment energy, in the range 900–1000 °C, and characterized them usi...
Autores principales: | , , , , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Nature Publishing Group
2017
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5307965/ https://www.ncbi.nlm.nih.gov/pubmed/28195125 http://dx.doi.org/10.1038/srep42315 |
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author | Wang, Kun Doerner, R. P. Baldwin, M. J. Meyer, F. W. Bannister, M. E. Darbal, Amith Stroud, Robert Parish, Chad M. |
author_facet | Wang, Kun Doerner, R. P. Baldwin, M. J. Meyer, F. W. Bannister, M. E. Darbal, Amith Stroud, Robert Parish, Chad M. |
author_sort | Wang, Kun |
collection | PubMed |
description | Nanotendril “fuzz” will grow under He bombardment under tokamak-relevant conditions on tungsten plasma-facing materials in a magnetic fusion energy device. We have grown tungsten nanotendrils at low (50 eV) and high (12 keV) He bombardment energy, in the range 900–1000 °C, and characterized them using electron microscopy. Low energy tendrils are finer (~22 nm diameter) than high-energy tendrils (~176 nm diameter), and low-energy tendrils have a smoother surface than high-energy tendrils. Cavities were omnipresent and typically ~5–10 nm in size. Oxygen was present at tendril surfaces, but tendrils were all BCC tungsten metal. Electron diffraction measured tendril growth axes and grain boundary angle/axis pairs; no preferential growth axes or angle/axis pairs were observed, and low-energy fuzz grain boundaries tended to be high angle; high energy tendril grain boundaries were not observed. We speculate that the strong tendency to high-angle grain boundaries in the low-energy tendrils implies that as the tendrils twist or bend, strain must accumulate until nucleation of a grain boundary is favorable compared to further lattice rotation. The high-energy tendrils consisted of very large (>100 nm) grains compared to the tendril size, so the nature of the high energy irradiation must enable faster growth with less lattice rotation. |
format | Online Article Text |
id | pubmed-5307965 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2017 |
publisher | Nature Publishing Group |
record_format | MEDLINE/PubMed |
spelling | pubmed-53079652017-02-22 Morphologies of tungsten nanotendrils grown under helium exposure Wang, Kun Doerner, R. P. Baldwin, M. J. Meyer, F. W. Bannister, M. E. Darbal, Amith Stroud, Robert Parish, Chad M. Sci Rep Article Nanotendril “fuzz” will grow under He bombardment under tokamak-relevant conditions on tungsten plasma-facing materials in a magnetic fusion energy device. We have grown tungsten nanotendrils at low (50 eV) and high (12 keV) He bombardment energy, in the range 900–1000 °C, and characterized them using electron microscopy. Low energy tendrils are finer (~22 nm diameter) than high-energy tendrils (~176 nm diameter), and low-energy tendrils have a smoother surface than high-energy tendrils. Cavities were omnipresent and typically ~5–10 nm in size. Oxygen was present at tendril surfaces, but tendrils were all BCC tungsten metal. Electron diffraction measured tendril growth axes and grain boundary angle/axis pairs; no preferential growth axes or angle/axis pairs were observed, and low-energy fuzz grain boundaries tended to be high angle; high energy tendril grain boundaries were not observed. We speculate that the strong tendency to high-angle grain boundaries in the low-energy tendrils implies that as the tendrils twist or bend, strain must accumulate until nucleation of a grain boundary is favorable compared to further lattice rotation. The high-energy tendrils consisted of very large (>100 nm) grains compared to the tendril size, so the nature of the high energy irradiation must enable faster growth with less lattice rotation. Nature Publishing Group 2017-02-14 /pmc/articles/PMC5307965/ /pubmed/28195125 http://dx.doi.org/10.1038/srep42315 Text en Copyright © 2017, The Author(s) http://creativecommons.org/licenses/by/4.0/ This work is licensed under a Creative Commons Attribution 4.0 International License. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in the credit line; if the material is not included under the Creative Commons license, users will need to obtain permission from the license holder to reproduce the material. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/ |
spellingShingle | Article Wang, Kun Doerner, R. P. Baldwin, M. J. Meyer, F. W. Bannister, M. E. Darbal, Amith Stroud, Robert Parish, Chad M. Morphologies of tungsten nanotendrils grown under helium exposure |
title | Morphologies of tungsten nanotendrils grown under helium exposure |
title_full | Morphologies of tungsten nanotendrils grown under helium exposure |
title_fullStr | Morphologies of tungsten nanotendrils grown under helium exposure |
title_full_unstemmed | Morphologies of tungsten nanotendrils grown under helium exposure |
title_short | Morphologies of tungsten nanotendrils grown under helium exposure |
title_sort | morphologies of tungsten nanotendrils grown under helium exposure |
topic | Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5307965/ https://www.ncbi.nlm.nih.gov/pubmed/28195125 http://dx.doi.org/10.1038/srep42315 |
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