1997
DOI: 10.1016/s0022-3115(97)00256-0
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Primary damage formation in bcc iron

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Cited by 277 publications
(178 citation statements)
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References 18 publications
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“…Since there is a high density of interstitial atoms in the cases of SIA = 200 and SIA = 300, the result may imply that larger sized SIA clusters can be absorbed by the grain boundary more easily. This conclusion was consistent with the previous findings that the larger SIA clusters can show a higher mobility than the scattered point defects [46,51]. Most of the SIAs have been absorbed by the grain boundary after system relaxation for 50 ps at 300 K, resulting in the significant relaxation of the potential energy in the GB area.…”
Section: Simulation Methodssupporting
confidence: 93%
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“…Since there is a high density of interstitial atoms in the cases of SIA = 200 and SIA = 300, the result may imply that larger sized SIA clusters can be absorbed by the grain boundary more easily. This conclusion was consistent with the previous findings that the larger SIA clusters can show a higher mobility than the scattered point defects [46,51]. Most of the SIAs have been absorbed by the grain boundary after system relaxation for 50 ps at 300 K, resulting in the significant relaxation of the potential energy in the GB area.…”
Section: Simulation Methodssupporting
confidence: 93%
“…The result agrees with the previous MD simulations that were carried out on single crystal structures where SIAs tend to cluster under cascade damage conditions [44,45]. Compared to the vacancies, SIAs and their clusters have been seen to possess a much lower activation energy [46,47] and therefore have a higher glissile mobility [48][49][50]. The rapid movement of SIAs was evidenced in the current study where the SIAs were prone to aggregate at the grain boundary even in the short timescale simulation.…”
Section: Simulation Methodssupporting
confidence: 91%
“…On the other hand, for vacancies, a dominant spatial correlation is found at the fourth nearest neighbor distance (NN4). The correlation of vacancies at NN4 was also observed for displacement cascades in Fe [14]. From this analysis, we take NN3 and NN4 as the clustering cutoff for SIAs and vacancies, respectively and use this as a default through the remainder of this article.…”
Section: Defect Clusteringmentioning
confidence: 99%
“…The simulations can be done in the micro-canonical ensemble with PBCs as in, for instance, References 54 through 57 or at constant pressure. [48,58] At the beginning of the collision phase, the time-step has to be carefully monitored in order to keep the total energy constant. It is usually taken to be of the order of 10 À17 seconds and can be increased to 10 À15 seconds during the cooling of the cascade.…”
Section: And the Primary Damagementioning
confidence: 99%