Comparison of Rare Earth Refinement in 4130 and HY100

Solidification based grain refinement has gained wide interest by both researchers and industry. This method provides a route for refinement in processes where thermomechanical approaches are ineffective. Prior research into 4130 and HY100 found very different responses when rare earth additions wer...

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Main Author: Robert Tuttle
Format: Article
Language:English
Published: MDPI AG 2021-03-01
Series:Metals
Subjects:
Online Access:https://www.mdpi.com/2075-4701/11/4/540
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spelling doaj-0e08594e59c04c149821e9303d67f6c62021-03-27T00:02:42ZengMDPI AGMetals2075-47012021-03-011154054010.3390/met11040540Comparison of Rare Earth Refinement in 4130 and HY100Robert Tuttle0Mechanical Engineering Department, Saginaw Valley State University, University Center, Saginaw, MI 48710, USASolidification based grain refinement has gained wide interest by both researchers and industry. This method provides a route for refinement in processes where thermomechanical approaches are ineffective. Prior research into 4130 and HY100 found very different responses when rare earth additions were made. The 4130 was effectively refined while HY100 showed no response. The cause of this difference was not determined. The research presented in this paper examined heats of 4130 and HY100 with rare earth silicide or EGR additions. Characterization included macrostructure examination, mechanical testing, thermal analysis, and electron microscopy. Refinement was observed only in the treated 4130 heats and corresponded to an increase in the peritectic temperature. The HY100 heats had no changes in macrostructure or solidification reactions. Rare earth containing inclusions of similar compositions were observed in the treated 4130 and HY100 heats. These inclusions appear to be a good fit for austenite based on the 4130 data. It was proposed that the unresponsiveness of HY100 was due to the strong segregation of nickel before the peritectic in that alloy. Nickel promotes austenite, and its segregation may provide a stronger driving force for its formation than the energy barrier reduction caused by the presence of rare earth inclusions.https://www.mdpi.com/2075-4701/11/4/540solidificationgrain refinementthermal analysisrare earth
collection DOAJ
language English
format Article
sources DOAJ
author Robert Tuttle
spellingShingle Robert Tuttle
Comparison of Rare Earth Refinement in 4130 and HY100
Metals
solidification
grain refinement
thermal analysis
rare earth
author_facet Robert Tuttle
author_sort Robert Tuttle
title Comparison of Rare Earth Refinement in 4130 and HY100
title_short Comparison of Rare Earth Refinement in 4130 and HY100
title_full Comparison of Rare Earth Refinement in 4130 and HY100
title_fullStr Comparison of Rare Earth Refinement in 4130 and HY100
title_full_unstemmed Comparison of Rare Earth Refinement in 4130 and HY100
title_sort comparison of rare earth refinement in 4130 and hy100
publisher MDPI AG
series Metals
issn 2075-4701
publishDate 2021-03-01
description Solidification based grain refinement has gained wide interest by both researchers and industry. This method provides a route for refinement in processes where thermomechanical approaches are ineffective. Prior research into 4130 and HY100 found very different responses when rare earth additions were made. The 4130 was effectively refined while HY100 showed no response. The cause of this difference was not determined. The research presented in this paper examined heats of 4130 and HY100 with rare earth silicide or EGR additions. Characterization included macrostructure examination, mechanical testing, thermal analysis, and electron microscopy. Refinement was observed only in the treated 4130 heats and corresponded to an increase in the peritectic temperature. The HY100 heats had no changes in macrostructure or solidification reactions. Rare earth containing inclusions of similar compositions were observed in the treated 4130 and HY100 heats. These inclusions appear to be a good fit for austenite based on the 4130 data. It was proposed that the unresponsiveness of HY100 was due to the strong segregation of nickel before the peritectic in that alloy. Nickel promotes austenite, and its segregation may provide a stronger driving force for its formation than the energy barrier reduction caused by the presence of rare earth inclusions.
topic solidification
grain refinement
thermal analysis
rare earth
url https://www.mdpi.com/2075-4701/11/4/540
work_keys_str_mv AT roberttuttle comparisonofrareearthrefinementin4130andhy100
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