Segregation and Ordering of Light Interstitials (B, C, H, and N) in Cr-Ni Alloys: Implications for Grain Boundary Stability in Superalloy Design
Tyler D. Dole\v{z}al, Rodrigo Freitas, Ju Li

TL;DR
This study uses Monte Carlo simulations to analyze how light interstitials like B, C, and N affect grain boundary stability and hydrogen behavior in Cr-Ni alloys, providing insights for superalloy design.
Contribution
It offers a computational framework revealing the segregation, ordering, and effects of light interstitials on grain boundary stability and hydrogen embrittlement mitigation in superalloys.
Findings
Boron prefers grain boundaries and stabilizes them.
Carbon and nitrogen form precipitates and have limited GB solubility.
Hydrogen tends to migrate inward along Cr- and Ni-rich GBs, avoiding Mo-enriched regions.
Abstract
The segregation and ordering behavior of light interstitials (B, C, and N) in Cr30-Ni is examined, as these elements are critical for grain boundary stability and high-temperature mechanical performance in Ni-based superalloys. Using Monte Carlo simulations, we identify the chemical and structural preferences of these interstitials in both bulk and grain boundary (GB) environments, aligning with experimental segregation and precipitation trends. Boron strongly prefers GBs over the bulk, where it enhances GB cohesion and stabilizes the GB structure. Uniquely, boron induces a structural transformation at higher concentrations, hinting at the formation of serrated GBs where boron content is high, which improves high-temperature mechanical performance. Carbon and nitrogen form carbide and nitride motifs and exhibit limited GB solubility, reinforcing their precipitation tendencies. In…
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