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X-ray diffraction from shock driven Sn microjets

机译:冲击驱动Sn微射流的X射线衍射

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摘要

In situ x-ray diffraction was performed on shock-generated microjets composed of Sn and Sn-4Ag. Under low pressure drives (similar to 21 GPa), a significant fraction of the jet volume was found to be in the beta - Sn phase, and these crystallites were much smaller than the initial grain size of the material. Significant quantities of amorphous (molten) material were observed for higher drive pressures (similar to 25-35 GPa). The extent of melting at these pressures was greater than would be predicted for uniaxial shock loading. Diffraction patterns from the Sn-4Ag alloy showed a peak that is consistent with the expected Ag3Sn intermetallic phase. This peak remained evident under drive conditions where the sample was otherwise fully amorphous. This indicates a slushy or a mixed phase of liquid Sn and solid Ag3Sn. Given the eutectic character of this alloy, this observation is attributed to a kinetic limitation on the dissolution of Ag3Sn. This implies that a much broader range of drive conditions will lead to mixed phase jets and ejecta than would be predicted from the equilibrium melt boundary of such alloys. Published under an exclusive license by AIP Publishing.
机译:对由Sn和Sn-4Ag组成的冲击产生的微射流进行了原位X射线衍射。在低压驱动(类似于21 GPa)下,发现射流体积的很大一部分处于β-Sn相,并且这些微晶远小于材料的初始晶粒尺寸。在较高的驱动压力(类似于 25-35 GPa)下观察到大量非晶态(熔融)材料。在这些压力下的熔化程度大于单轴冲击载荷的预测程度。Sn-4Ag合金的衍射图显示出与预期的Ag3Sn金属间相一致的峰。在样品完全无定形的驱动条件下,该峰仍然很明显。这表明液态 Sn 和固体 Ag3Sn 的泥浆相或混合相。鉴于该合金的共晶特性,这一观察结果归因于Ag3Sn溶解的动力学限制。这意味着,与从此类合金的平衡熔体边界预测的相比,更广泛的驱动条件将导致混合相射流和喷射。在 AIP Publishing 的独家许可下发布。

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