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The total stress approach to martensitic transformations in Ti-Nb-based alloys.

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Peer-reviewed

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Abstract

Metastable β Ti alloys have potential for vibration damping and actuation applications within the aerospace industry due to thermal and mechanical hysteresis. However, variations in transformation parameters, which are also seen to change following thermal or mechanical cycling, significantly limit industrial acceptance. There is a widespread belief that these variations are a consequence of ⍵ phase formation. However, here we provide evidence to show that this is not necessarily the case. Instead, we show how residual stresses and defect structures are crucial to the transformation of these alloys and present an understanding of the mechanism that governs their behaviour. Importantly, we highlight the consequences for the design of new transforming alloys and component geometries, and how current design theories may need to be employed in conjunction with other methods to effectively prevent longer-term changes in behaviour. To this end, we demonstrate how functional properties could be periodically recovered by introducing short intercycle heat treatments and suggest possible next steps for advancing our understanding of these materials.

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Acknowledgements: The authors would like to acknowledge Diamond Light Source for the provision of beam time under MG30411, MG33585, and MG33592, and to Dr Stefan Michalik for his assistance. Support from the EPSRC under EP/R511870/1 and EP/R513180/1 is also appreciated. We also acknowledge the support of the Wolfson Electron Microscopy Suite at the University of Cambridge and the ThermoFisher Spectra 300 TEM, funded by EPSRC under grant EP/R008779/1.

Journal Title

Commun Mater

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Journal ISSN

2662-4443
2662-4443

Volume Title

6

Publisher

Springer Nature

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Except where otherwised noted, this item's license is described as http://creativecommons.org/licenses/by/4.0/
Sponsorship
Engineering and Physical Sciences Research Council (EP/R008779/1)
EPSRC (EP/R513180/1)
Engineering and Physical Sciences Research Council (EP/R511870/1)
The authors would like acknowledge Diamond Light Source for the provision of beam time under MG30411, MG33585 and MG33592. Support from the EPSRC under EP/R511870/1 and EP/R513180/1 is also appreciated. We also acknowledge the support of the Wolfson Electron Microscopy Suite at the University of Cambridge and the ThermoFisher Spectra 300 TEM funded by EPSRC under grant EP/R008779/1.

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