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Phase chemistry and precipitation reactions in maraging steels: Part 4. Discussion and conclusions

Journal Article · · Metallurgical Transactions, A (Physical Metallurgy and Materials Science); (United States)
DOI:https://doi.org/10.1007/BF02668193· OSTI ID:6209515
 [1]; ;  [2]
  1. Cambridge Univ. (United Kingdom). Department of Materials Science and Metallurgy
  2. Univ. of Oxford (United Kingdom). Department of Materials
This article summarizes studies of phase chemistry and precipitation reactions in a variety of maraging steels. The roles of different phases and alloying elements are investigated by comparing the behavior of different steels. The phases considered are Ni[sub 3]Ti, Fe[sub 7]Mo[sub 6] [mu] phase, Fe[sub 2]Mo Laves phase, [omega] phase, Ti[sub 6]Si[sub 7]Ni[sub 16]G phase, Z phase, austenite, and [alpha] matrix. The alloying elements discussed are Ti, Al, Mo, Si, Mn, Ni, Cr, and Co. By comparing the aging behavior of both commercial steels and model alloys, a major role of Co is confirmed to be the lowering of the matrix solubility of Mo. Of the two main hardening elements in maraging steels (namely, Ti and Mo), Ti is much more active than Mo in the very early stage of precipitation. The main Mo-rich precipitate found in this work was Fe[sub 7]Mo[sub 6][mu] phase instead of Laves phase. The precipitation of Mo is modified by the presence of Ti. [omega] phase appears only in Ti-free alloys, especially when aged at a low temperature. The quantity of Ni-containing precipitates and the presence of Cr in the steels change the austenite reversion behavior. Other phases, such as G phase and Z phase, contribute to age hardening in different types of maraging alloys.
OSTI ID:
6209515
Journal Information:
Metallurgical Transactions, A (Physical Metallurgy and Materials Science); (United States), Journal Name: Metallurgical Transactions, A (Physical Metallurgy and Materials Science); (United States) Vol. 24A:6; ISSN 0360-2133; ISSN MTTABN
Country of Publication:
United States
Language:
English