This is a page describing data taken during an experiment at the ISIS Neutron and Muon Source. Information about the ISIS Neutron and Muon Source can be found at https://www.isis.stfc.ac.uk.
In-situ study of nanoscale omega phase kinetics in beta Ti alloys as a function of quenching rate
Abstract: This work aims to understand the precipitation behaviour of nanoscale omega phase in beta phase matrix of Ti alloys as a function of quenching rate. The omega phase is regarded as the potent nucleant site for alpha phase precipitate, which is considered to strengthen Ti alloys. This study will help us optimising omega phase precipitates, which in turn will help in controlling alpha phase precipitation to achieve higher strength. This study will also enable us to quantify microstructure by deconvoluting size, volume fraction and elemental partitioning of omega phase. Additionally, outputs of this study can be used to optimise the quenching rate for obtaining next-generation high strength beta Ti alloy. Optimising quenching rate will create an impact on aerospace industry for structural applications as thickness of material is compromised with quenching rate for achieving higher strength
Principal Investigator: Professor Bo Chen
Experimenter: Dr David Parfitt
Experimenter: Dr Gokulnath Kadavath
Experimenter: Mr Hitesh Sharma
Local Contact: Dr Diego Alba Venero
Experimenter: Mr Deepak Sharma
DOI: 10.5286/ISIS.E.RB1820495
ISIS Experiment Number: RB1820495
Part DOI | Instrument | Public release date | Download Link |
---|---|---|---|
10.5286/ISIS.E.99686963 | LARMOR | 16 November 2021 | Download |
Publisher: STFC ISIS Neutron and Muon Source
Data format: RAW/Nexus
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Data Citation
The recommended format for citing this dataset in a research
publication is as:
[author], [date], [title], [publisher],
[doi]
For Example:
Professor Bo Chen et al; (2018): In-situ study of nanoscale omega phase kinetics in beta Ti alloys as a function of quenching rate, STFC ISIS Neutron and Muon Source, https://doi.org/10.5286/ISIS.E.RB1820495
Data is released under the CC-BY-4.0 license.