2015
DOI: 10.1016/j.ultramic.2015.05.013
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Characterisation of interfacial segregation to Cu-enriched precipitates in two thermally aged reactor pressure vessel steel welds

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Cited by 32 publications
(20 citation statements)
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“…Previous thermodynamic models suggested that in addition to enriching the Cu core, solutes such as Mn, Ni and Si form a surrounding shell due to reduction of the high interfacial energy between Fe and Cu [18]. Such core-shell structures were subsequently widely reported in APT studies, both under irradiation and thermal aging conditions [16,[19][20][21]. More recently, APT showed that at longer times (or higher irradiation fluence) after Cu in matrix is depleted, and when more Mn, Ni and Si atoms come out of solution, the core-shell structure gives way to a Cu-core-MnNiSi-appendage co-precipitate morphology.…”
Section: Introductionmentioning
confidence: 94%
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“…Previous thermodynamic models suggested that in addition to enriching the Cu core, solutes such as Mn, Ni and Si form a surrounding shell due to reduction of the high interfacial energy between Fe and Cu [18]. Such core-shell structures were subsequently widely reported in APT studies, both under irradiation and thermal aging conditions [16,[19][20][21]. More recently, APT showed that at longer times (or higher irradiation fluence) after Cu in matrix is depleted, and when more Mn, Ni and Si atoms come out of solution, the core-shell structure gives way to a Cu-core-MnNiSi-appendage co-precipitate morphology.…”
Section: Introductionmentioning
confidence: 94%
“…By coupling recent advances in near-atomic resolution characterization techniques in three dimensions, such as atom probe tomography (APT) [11,12], with atomistic simulation tools such as kinetic lattice Monte Carlo (KLMC) [13], it is possible to study the precipitation pathways of multicomponent alloys in a quantitative manner. Here, we use these techniques to model the pathway of Cu-MnNiSi co-precipitation observed in irradiated (and thermally aged) Cu-bearing low-alloy steels [14][15][16]. Specifically, we focus on the mechanism of a transition of the coprecipitate from a Cu-core-MnNiSi-shell structure to a Cu-core-MnNiSi-appendage structure.…”
Section: Introductionmentioning
confidence: 99%
“…The latter result has been confirmed on RPV steels (e.g., [58]). -Long term aging (up to 100,000 hours) at 330°C on high Cu steels (Cu > 0.4 wt%) leads to the formation of Cu-rich precipitates made of a Cu-rich core surrounded by a shell of Mn, Ni and Si atoms, very similar to clusters obtained after neutron irradiation [134,135].…”
Section: Hardening Defectsmentioning
confidence: 68%
“…More specifically, several analyses showed that Ni, Mn, and Si reduce the interface energy of Cu clusters in Fe (e.g., [85,135]), which supports the formation of Ni, Mn, and Si shells around Cu-rich cores.…”
Section: Hardening Defectsmentioning
confidence: 95%
“…The Cu content in modern Grade 3 A508 RPV steels is low (typically < 0.1 at %), and Cu phase separates early in the lifetime of the reactor (<10 23 n m -2 fluence, ≥1 MeV) [69]. Due to the established flux-coupling effect of vacancy drag of Ni, Mn and Si to existing Cu clusters [3,27,70] and the strong binding energy (-0.2 eV) of Cu-Ni-Mn triplets, existing Cu clusters will act locally as nucleation points for Mn-Ni clusters, evidence for this is seen experimentally with the observation of Cu-rich cores surrounded by Mn-Ni-Si rich shells [5,[36][37][38]71]. The availability of Si (0.2 -0.6 at.…”
Section: Mn-ni Tripletsmentioning
confidence: 96%