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Direct observation of the dynamic evolution of precipitates in aluminium alloy 7021 at high strain rates via high energy synchrotron X-rays

dc.contributor.authorMirihanage, W.U
dc.contributor.authorRobson, J.D
dc.contributor.authorMishra, S
dc.contributor.authorHidalgo-Manrique, P
dc.contributor.authorQuinta da Fonseca, J
dc.contributor.authorDaniel, C.S
dc.contributor.authorPrangnell, P.B
dc.contributor.authorMichalik, S
dc.contributor.authorMagdysyuk, O.V
dc.contributor.authorConnolley, T
dc.contributor.authorDrakopoulus, M
dc.date.accessioned2023-12-22T08:45:06Z
dc.date.available2023-12-22T08:45:06Z
dc.date.issued2020-12-02
dc.identifier.citationW.U. Mirihanage, J.D. Robson, S. Mishra, P. Hidalgo-Manrique, J. Quinta da Fonseca, C.S. Daniel, P.B. Prangnell, S. Michalik, O.V. Magdysyuk, T. Connolley, M. Drakopoulos, Direct observation of the dynamic evolution of precipitates in aluminium alloy 7021 at high strain rates via high energy synchrotron X-rays, Acta Materialia, Volume 205, 2021, 116532, ISSN 1359-6454, https://doi.org/10.1016/j.actamat.2020.116532. (https://www.sciencedirect.com/science/article/pii/S1359645420309691)es
dc.identifier.issn1359-6454
dc.identifier.urihttps://hdl.handle.net/10115/27722
dc.descriptionThe EPSRC are thanked for financial support through the associated programme grant LightFORM (EP/R001715/1) and EP/P02680X/1. Diamond Light Source (UK) is acknowledged for granting beam time to undertake the experiments at beamline I12 (EE13828). P.B. Prangnell is grateful to the Royal Academy of Engi neering, UK, and Airbus for financial support through the Airbus-University of Manchester Centre for Metallurgical Excellence.es
dc.description.abstractAn improved understanding of the phenomenon of dynamic precipitation is important to accurately model and simulate many industrial manufacturing processes with high strength Al-alloys. Dynamic ageing in 7xxx Al-alloys can occur as a result of both the strain and heat. Small angle X-ray scattering (SAXS) is an advanced technique that allows the precipitation processes to be studied in situ, but to date this has only been possible at lower than industrially relevant strain rates (e.g. < 10−3). In this contribution, we demonstrate the potential of in-situ SAXS studies of metallic alloys at higher strain rates (10−2) than previously, using a high energy synchrotron X-ray. The time resolved SAXS information has been used to evaluate dynamic precipitate evolution models and has demonstrated that at high strain rates a new regime must be considered which includes the more significant effect of vacancy annihilation, leading to a clear strain rate, rather than just strain, kinetic dependence.es
dc.language.isoenges
dc.publisherElsevieres
dc.rightsAtribución 4.0 Internacional*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/*
dc.subjecthigh-strength aluminium alloyses
dc.subjectdynamic ageinges
dc.subjectsmall angle X-ray scattering (SAXS)es
dc.subjectin-situ precipitation characterisationes
dc.titleDirect observation of the dynamic evolution of precipitates in aluminium alloy 7021 at high strain rates via high energy synchrotron X-rayses
dc.typeinfo:eu-repo/semantics/articlees
dc.identifier.doi10.1016/j.actamat.2020.116532es
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses


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Atribución 4.0 InternacionalExcept where otherwise noted, this item's license is described as Atribución 4.0 Internacional