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Microstructural Evolution and Age Hardening in Aluminium Alloys ...

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<strong>Microstructural</strong> <strong>Evolution</strong> <strong>in</strong> <strong>Age</strong>d Al <strong>Alloys</strong> 103EX (400kV), <strong>and</strong> a JEOL ARM operat<strong>in</strong>g at600kV.Al-Cu BASED ALLOYSThe most widely studied age-harden<strong>in</strong>g alloysystem is Al–Cu, <strong>and</strong> several commercialalloys based on this system rema<strong>in</strong> <strong>in</strong>use <strong>in</strong> the 2xxx alloy series. Although thealloy is composed of only two elements, themicrostructural evolution is complex, <strong>and</strong>the precipitation sequence varies depend<strong>in</strong>gon the degree of supersaturation <strong>and</strong>the ag<strong>in</strong>g temperature. Figure 1 shows theAl-rich corner of the equilibrium Al–Cuphase diagram, <strong>and</strong> <strong>in</strong>cludes the metastablesolvus boundaries for GP zones, <strong>and</strong>. Over many studies [9–29], it has beenproposed that the decomposition sequence<strong>in</strong> this system conta<strong>in</strong>s one or more of thefollow<strong>in</strong>g processes:Supersaturated Solid Solution ( SSSS)→GP zones →θ'' →θ' →θThe complete precipitation sequence canonly occur when the alloy is aged at tem-peratures below the GP zone solvus (Fig.1). Various steps <strong>in</strong> this process may besuppressed by ag<strong>in</strong>g at temperatures closeto or above the <strong>in</strong>termediate solvus temperatures.Figure 2 shows a hardness–timeplot for Al–1.7Cu-aged at 130 <strong>and</strong> 190C,which represents temperatures below <strong>and</strong>above the GP zone solvus temperature, respectively.The first stage of harden<strong>in</strong>g at130C is attributed to the formation of GPzones. After reach<strong>in</strong>g a critical diameter ofbetween 5 <strong>and</strong> 10nm, an <strong>in</strong>cubation periodcommences, dur<strong>in</strong>g which the zone size<strong>and</strong> the hardness rema<strong>in</strong> constant [15–17].Further ag<strong>in</strong>g results <strong>in</strong> a second rise <strong>in</strong>hardness, attributed to precipitation. Theformation of is also followed by a shorter<strong>in</strong>cubation period <strong>and</strong> the subsequent formationof the metastable phase. Prolongedag<strong>in</strong>g results <strong>in</strong> the formation of theequilibrium phase. Each precipitationstage does not necessarily correspond tothe stages observed <strong>in</strong> the hardness curve,<strong>and</strong> more than two phases can coexist at agiven stage of the ag<strong>in</strong>g process. The mechanismof the transformation sequence fromone phase to another usually <strong>in</strong>volves heterogeneousnucleation at the sites of earlierproducts, result<strong>in</strong>g <strong>in</strong> f<strong>in</strong>e <strong>and</strong> uniform precipitatedispersions. However, under a suitabledegree of supersaturation, the products<strong>in</strong> the above evolutionary sequencenucleate directly <strong>in</strong>to the matrix [17]. ThisFIG. 1. Al-rich corner of the Al–Cu phase diagramshow<strong>in</strong>g the metastable solvus boundaries for GPzones, <strong>and</strong> , together with the equilibrium solvusl<strong>in</strong>e for the phase. After Beton <strong>and</strong> Rollason [20] <strong>and</strong>Murray [21].FIG. 2. Hardness–time plot for Al–1.7Cu aged at 130<strong>and</strong> 190C, show<strong>in</strong>g the effect of a 0.01 Sn addition.After Hardy [16].

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