Experimental study reveals that high temperatures and slow cooling promote interfacial Mg2Si precipitation in AA6061 cladding, highlighting parameters to optimize nuclear fuel integrity.
Understanding microstructural evolution at the hot isostatically pressed (HIP) cladding AA6061/AA6061 interface is essential for advancing the Zr-laminated U10Mo monolithic fuel system for research and test reactors. In this study, AA6061 plates were diffusion bonded via HIP at two temperatures (450 and 560 °C) and two cooling rates (1 and 45 °C/min). Scanning electron microscopy and quantitative image analysis were conducted to characterize the Mg 2 Si precipitation, with an emphasis on precipitate linear density and size at the AA6061/AA6061 HIP-bonded interface. The results revealed a pronounced accumulation of Mg 2 Si precipitates at the AA6061/AA6061 interface, with the highest precipitate density and largest precipitate size occurring in samples HIP-processed at 560 °C followed by slow cooling. Post-HIP heat treatment experiments demonstrated that water quenching after solutionizing effectively suppressed Mg 2 Si precipitation at the interface. To evaluate the feasibility of applying such post-HIP heat treatments within the full monolithic fuel system, simple growth kinetics estimates were conducted for the Zr/AA6061 and U–Mo/Zr interfaces. Overall, these findings provide valuable guidance for optimizing HIP parameters and potential post-HIP treatments to enhance the structural integrity and performance of monolithic fuel cladding.
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Pido et al. (2026) studied this question.
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