“…The Ag-Mg-Ca ternary and Ag-Mg-Ca-Cu quaternary systems were selected for detailed analysis, since: (i) all elements have simple electronic structures and are thermodynamically compatible, forming multiple deep binary eutectics and relatively low temperature intermetallics with relatively similar negative (with the exception of Ag-Cu) heats of mixing (dependent on composition); (ii) each of the constituent elements display a large difference in atomic radius and the required specific radius ratios favoured for glass formation (Cu -128 pm, Ag -144 pm, Mg -160 pm, and Ca -196 pm), which geometrically allows for a larger compositional range of efficiently packed clusters [3,4], and (iii) glass formation in the binary Ag-Ca system has been reported over a broad composition range [5] and high GFA in the Ca-rich region of both the Ag-Mg-Ca ternary and Ag-Mg-Ca-Cu quaternary system has been confirmed by Amiya and Inoue [6], with the Ca 60 Mg 20 Ag 20 and Ca 60 Mg 20 Ag 10 Cu 10 alloys exhibiting a critical casting diameter (D C ) of 4 and 7 mm, respectively. Copper was specifically selected for this work as it too has exceptionally high electrical and thermal conductivity and has a similar, simple electronic configuration to Ag with a full d-electron shell and single s-electron in its outer shell.…”