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“Influence of Si, Sb and Sr Additions on the Microstructure ...

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x Chapter 4: Results <str<strong>on</strong>g>and</str<strong>on</strong>g> Discussi<strong>on</strong><br />

higher hardness obtained with <str<strong>on</strong>g>Si</str<strong>on</strong>g> <str<strong>on</strong>g>and</str<strong>on</strong>g> <str<strong>on</strong>g>Sb</str<strong>on</strong>g> additi<strong>on</strong> at peak aged c<strong>on</strong>diti<strong>on</strong> might also be<br />

attributed to <strong>the</strong> presence <str<strong>on</strong>g>of</str<strong>on</strong>g> more number <str<strong>on</strong>g>of</str<strong>on</strong>g> c<strong>on</strong>tinuous precipitates.<br />

It is found from <strong>the</strong> aged microstructure <str<strong>on</strong>g>of</str<strong>on</strong>g> <str<strong>on</strong>g>Sr</str<strong>on</strong>g> added alloy that more amounts<br />

<str<strong>on</strong>g>of</str<strong>on</strong>g> disc<strong>on</strong>tinuous precipitate forms in <strong>the</strong> initial stage <str<strong>on</strong>g>of</str<strong>on</strong>g> ageing. More number <str<strong>on</strong>g>of</str<strong>on</strong>g><br />

boundaries is seen with DP compared to o<strong>the</strong>r alloys as shown in Figure 4.36 (d). The<br />

volume fracti<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> disc<strong>on</strong>tinuous precipitates calculated is slightly higher / equal<br />

compared to <strong>the</strong> base alloy (ref. Table 4.4). It could be also seen from Table 4.3 that<br />

<str<strong>on</strong>g>Sr</str<strong>on</strong>g> added alloy reaches <strong>the</strong> peak hardness little early than <strong>the</strong> base alloy. This is due to<br />

low amount <str<strong>on</strong>g>of</str<strong>on</strong>g> Al available in <strong>the</strong> solid soluti<strong>on</strong>. Nussbaum et al [238] <str<strong>on</strong>g>and</str<strong>on</strong>g> Lee et al<br />

[231] reported that <str<strong>on</strong>g>Sr</str<strong>on</strong>g> modifies <strong>the</strong> precipitati<strong>on</strong> behavior <str<strong>on</strong>g>of</str<strong>on</strong>g> Mg-Al alloys by<br />

promoting more precipitates al<strong>on</strong>g <strong>the</strong> grain boundaries. However, <strong>the</strong> reas<strong>on</strong> behind<br />

_ such occurrence is not known. On <strong>the</strong> o<strong>the</strong>r h<str<strong>on</strong>g>and</str<strong>on</strong>g> <strong>the</strong> formati<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> DP during ageing<br />

<str<strong>on</strong>g>of</str<strong>on</strong>g> Mg-Al is a combined effect <str<strong>on</strong>g>of</str<strong>on</strong>g> Al in <strong>the</strong> solid soluti<strong>on</strong>, grain size <str<strong>on</strong>g>and</str<strong>on</strong>g> ageing<br />

temperature [I46]. High amount <str<strong>on</strong>g>of</str<strong>on</strong>g> Al, finer grain size (high angle grain boundary)<br />

<str<strong>on</strong>g>and</str<strong>on</strong>g> medium ageing temperature (I50-250°C) leads to more DP in Mg-Al alloys.<br />

Hence, <strong>the</strong> boundary characterizati<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> <str<strong>on</strong>g>Sr</str<strong>on</strong>g> added alloy is necessary to underst<str<strong>on</strong>g>and</str<strong>on</strong>g> <strong>the</strong><br />

precipitati<strong>on</strong> mechanism.<br />

Table 4.4: Volume fracti<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g> disc<strong>on</strong>tinuous precipitates formed in 120 min aged<br />

Samples<br />

Volume 4 i W<br />

fracti<strong>on</strong> <str<strong>on</strong>g>of</str<strong>on</strong>g><br />

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­ Allo AZ91 4 . ' 4 ' A AZ91+0.5%<str<strong>on</strong>g>Sr</str<strong>on</strong>g> ­<br />

L g Y ._ X %si _ . g <str<strong>on</strong>g>Sb</str<strong>on</strong>g> g i<str<strong>on</strong>g>Si</str<strong>on</strong>g>+0.2% <str<strong>on</strong>g>Sb</str<strong>on</strong>g><br />

disc<strong>on</strong>tinuous y 8.51:4 2.7i2.Z 4.l¢3.6 » l0.2¢5.2 3.5:l:2.8<br />

precipitates,<br />

% .<br />

4 AZ91+05 Az91+o 5% it 4 P Az91+o.5°/<br />

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