CONDENSED MATTER: STRUCTURAL, MECHANICAL, AND THERMAL PROPERTIES |
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Effect of microstructure on 3He migration in TiT1.9 films |
Haifeng Wang(王海峰), Shuming Peng(彭述明), Wei Ding(丁伟), Huahai Shen(申华海), Weidu Wang(王维笃), Xiaosong Zhou(周晓松), Xinggui Long(龙兴贵) |
Institute of Nuclear Physics and Chemistry, China Academy of Engineering Physics, Mianyang 621900, China |
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Abstract Two kinds of films were prepared to study the effect of microstructure on helium migration in Ti tritides. Both films showed different release behaviors and helium bubble distributions. In the film consisting of columnar grains, a two-layered structure was observed. Inclusions with a strip feature were found at the grain boundary, and no helium bubbles were distributed in these inclusions. However, helium preferred to migrate to the boundaries of these inclusions. Bubble linkage as a ribbon-like feature developed parallel to the film surface in the film consisting of columnar grains. More cracks were developed at the grain boundaries of the film consisting of columnar grains, although the helium content in the film consisting of columnar grains was less than that in the film consisting of equiaxed grains. A surface region with a small number of bubbles, or “depleted zone”, was observed near the surface. The cracks extending to the film surface were the pathways of the critical helium released from the film. The helium migration was strongly influenced by the grain microstructure.
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Received: 11 March 2018
Revised: 27 May 2018
Accepted manuscript online:
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PACS:
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61.72.Qq
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(Microscopic defects (voids, inclusions, etc.))
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81.40.Wx
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(Radiation treatment)
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68.55.-a
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(Thin film structure and morphology)
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Corresponding Authors:
Shuming Peng
E-mail: pengshuming@caep.cn
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Cite this article:
Haifeng Wang(王海峰), Shuming Peng(彭述明), Wei Ding(丁伟), Huahai Shen(申华海), Weidu Wang(王维笃), Xiaosong Zhou(周晓松), Xinggui Long(龙兴贵) Effect of microstructure on 3He migration in TiT1.9 films 2018 Chin. Phys. B 27 096103
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[1] |
Beavis L C and Kass W J 1977 J. Vac. Sci. Technol. 14 509
|
[2] |
Ding W, Long X G and Liang J H 2008 At. Engergy Sci. Technol 42 944 (in Chinese)
|
[3] |
Snow C S, Brewer L N, Gelles D S, Rodrguez M A, Kotula P G, Banks J C, Mangan M A and Browning J F 2008 J. Nucl. Mater. 374 147
|
[4] |
Chen R C, Yang L and Dai Y Y 2012 Chin. Phys. B 21 056601
|
[5] |
Zu X T, Yang L, Gao F, Peng S M, Heinisch H L, Long X G and Kurtz R J 2009 Phys. Rev. B 80 054104
|
[6] |
Zhang B L, Wang J and Hou Q 2011 Chin. Phys. B 20 036105
|
[7] |
Gong H F, Yan Y, Zhang X S, Lv W, Liu T and Ren Q S 2017 Chin. Phys. B 26 093104
|
[8] |
Thiébaut S, Décamps B, Pénisson J M, Limacher B, and Guégan A Percheron 2000 J. Nucl. Mater. 277 217
|
[9] |
Schober T, Trinkaus H and Lässer R 1986 J. Nucl. Mater. 141 453
|
[10] |
Bond G M, Browning J F and Snow C S 2010 J. Appl. Phys. 107 083514
|
[11] |
Snow C S, Browning J F, Bond G M, Rodriguez M A and Knapp J A 2014 J. Nucl. Mater. 453 296
|
[12] |
Trinkaus H and Singh B N 2003 J. Nucl. Mater. 323 229
|
[13] |
Gao X, Luo P and Chang H L 2015 Chin. Phys. Lett. 32 76101
|
[14] |
Chen M 2011 Acta Phys. Sin. 60 126602 (in Chinese)
|
[15] |
Parish C M, Snow C S, Kammler D R and Brewer L N 2010 J. Nucl. Mat. 403 191
|
[16] |
Parish C M, Snow C S, and Brewer L N 2009 J. Mater. Res. 24 1868
|
[17] |
Liang L, Tan X H, Xiang W, Wang Y, Cheng Y L and Ma M W 2015 Acta Phys. Sin. 64 046103 (in Chinese)
|
[18] |
Zhou Y L, Deng A H, Li R S, Zhang B L and Hou Q 2011 Acta Phys. Sin. 60 046604 (in Chinese)
|
[19] |
Shen H H, Peng S M, Long X G, Zhou X S, Yang L, Liu J H, Sun Q Q and Zu X T 2012 Chin. Phys. B 21 076101
|
[20] |
Shen H H, Peng S M, Long X G, Zhou X S, Yang L and Zu X T 2012 Vacuum 86 1097
|
[21] |
Savaloni H, Player M A, Gu E and Marr G V 1992 Vacuum 43 965
|
[22] |
Peng S M, Shen H H, Long X G, Zhou X S, Yang L and Zu X T 2012 Acta Phys. Sin. 61 176106
|
[23] |
Shen H H, Zu H Y, Peng S M, Yang L, Zhou X S, Sun K, Xiang X and Zu X T 2013 Mater. Lett. 106 259
|
[24] |
Savaloni H, Taherizadeh A and Zendehnam A 2004 Physica B 349 44
|
[25] |
Guo D C, Jiang X D, Huang J, Wang F R, Liu H J, Xiang X, Yang G X, Zheng W G and Zu X T 2014 Opt. Express 22 29020
|
[26] |
Zhou X S, Long, X G and Peng S M 2010 J.Nucl.Mater. 396 223
|
[27] |
Savaloni H and Player M A 1995 Vacuum 46 167
|
[28] |
Trinkaus H 1986 Radiat. Eff. 101 91
|
[29] |
Schober T and Farrell K 1989 J. Nucl. Mater. 168 171
|
[30] |
Schroeder H 1989 J. Nucl. Mater. 155-157 1032
|
[31] |
Chen J, Hung P and Trinkaus H 2000 Phys. Rev. B 61 12923
|
[32] |
Singh B N, Leffers T and Green W V 1984 J. Nucl. Mater. 125 287
|
[33] |
Grobenor C R M, Hentzell H T G and Smith D A 1984 Acta Metall. 32 773
|
[34] |
Rodriguez M A, Browning J F and Frazer C S 2007 Powder Diffr. 22 118
|
[35] |
Beavis L C and Miglionico C J 1972 J. Less-Common Met. 27 201
|
[36] |
Schober T and Trinkaus H 1991 J. Appl. Phys. 70 729
|
[37] |
Schober T and Trinkaus H 1990 J. Appl. Phys. 67 7587
|
[38] |
Mitchell D J and Provo J L 1985 J. Appl. Phys. 57 1855
|
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