Cascade fragmentation: deviation from power law in primary radiation damage
The sizes of defect clusters, produced in materials by energetic ion or neutron impacts, are critically important input for models describing microstructural evolution of irradiated materials. We propose a model for the distribution of sizes of vacancy and self-interstitial defect clusters formed by...
Ausführliche Beschreibung
Autor*in: |
A. E. Sand [verfasserIn] D. R. Mason [verfasserIn] A. De Backer [verfasserIn] X. Yi [verfasserIn] S. L. Dudarev [verfasserIn] K. Nordlund [verfasserIn] |
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Englisch |
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2017 |
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In: Materials Research Letters - Taylor & Francis Group, 2017, 5(2017), 5, Seite 357-363 |
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Übergeordnetes Werk: |
volume:5 ; year:2017 ; number:5 ; pages:357-363 |
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DOI / URN: |
10.1080/21663831.2017.1294117 |
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DOAJ045503516 |
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10.1080/21663831.2017.1294117 doi (DE-627)DOAJ045503516 (DE-599)DOAJ8c22bbc116da4b9f8455a5f91d11162c DE-627 ger DE-627 rakwb eng TA401-492 A. E. Sand verfasserin aut Cascade fragmentation: deviation from power law in primary radiation damage 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The sizes of defect clusters, produced in materials by energetic ion or neutron impacts, are critically important input for models describing microstructural evolution of irradiated materials. We propose a model for the distribution of sizes of vacancy and self-interstitial defect clusters formed by high-energy impacts in tungsten, and provide new data from in situ ion irradiation experiments to validate the model. The model predicts the statistics of sub-cascade splitting and the resulting distribution of primary defects extending over the entire range of cluster sizes, and is able to provide initial conditions for quantitative multi-scale simulations of microstructural evolution. Atomistic simulations lattice defects tungsten radiation damage Materials of engineering and construction. Mechanics of materials D. R. Mason verfasserin aut A. De Backer verfasserin aut X. Yi verfasserin aut S. L. Dudarev verfasserin aut K. Nordlund verfasserin aut In Materials Research Letters Taylor & Francis Group, 2017 5(2017), 5, Seite 357-363 (DE-627)73656179X (DE-600)2703730-7 21663831 nnns volume:5 year:2017 number:5 pages:357-363 https://doi.org/10.1080/21663831.2017.1294117 kostenfrei https://doaj.org/article/8c22bbc116da4b9f8455a5f91d11162c kostenfrei http://dx.doi.org/10.1080/21663831.2017.1294117 kostenfrei https://doaj.org/toc/2166-3831 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ SSG-OLC-PHA GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 5 2017 5 357-363 |
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The sizes of defect clusters, produced in materials by energetic ion or neutron impacts, are critically important input for models describing microstructural evolution of irradiated materials. We propose a model for the distribution of sizes of vacancy and self-interstitial defect clusters formed by high-energy impacts in tungsten, and provide new data from in situ ion irradiation experiments to validate the model. The model predicts the statistics of sub-cascade splitting and the resulting distribution of primary defects extending over the entire range of cluster sizes, and is able to provide initial conditions for quantitative multi-scale simulations of microstructural evolution. |
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The sizes of defect clusters, produced in materials by energetic ion or neutron impacts, are critically important input for models describing microstructural evolution of irradiated materials. We propose a model for the distribution of sizes of vacancy and self-interstitial defect clusters formed by high-energy impacts in tungsten, and provide new data from in situ ion irradiation experiments to validate the model. The model predicts the statistics of sub-cascade splitting and the resulting distribution of primary defects extending over the entire range of cluster sizes, and is able to provide initial conditions for quantitative multi-scale simulations of microstructural evolution. |
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The sizes of defect clusters, produced in materials by energetic ion or neutron impacts, are critically important input for models describing microstructural evolution of irradiated materials. We propose a model for the distribution of sizes of vacancy and self-interstitial defect clusters formed by high-energy impacts in tungsten, and provide new data from in situ ion irradiation experiments to validate the model. The model predicts the statistics of sub-cascade splitting and the resulting distribution of primary defects extending over the entire range of cluster sizes, and is able to provide initial conditions for quantitative multi-scale simulations of microstructural evolution. |
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|
score |
7.401143 |