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Materials Science in Additive Manufacturing                           Heterostructures of A131 steel by DED




                         A                       B                       C













                         D                       E                       F













            Figure 9. Broken surface of the tensile sample of AB A131 steel: (A-C) SEM images of defects at the edge; and (D-F) SEM images of defects in the middle.
            (C, inset) EDS spectrums of the particle defect. Scale bars: 500 µm (A and D); 50 µm (B and E); 20 µm (C); 10 µm (F)
            Abbreviations: AB: As-built; SEM: Scanning electron microstructure; EDS: Energy dispersive spectrometer; O: Oxygen; Al: Aluminum; N: Nitrogen; Mn:
            Manganese

            along ND. The grains were relatively small and comprised   Figure 10G displays the microstructure at the interface
            columnar grains, fine acicular martensite, and some   between the single-pass track and the 304L steel substrate,
            equiaxed grains, attributed to dendritic growth during the   consisting  of equiaxed grains and  acicular  martensite.
            consolidation of the melt pool under rapid cooling rates.    A  distinctive interface could be observed, where fine
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            Discontinuous columnar crystals were formed along ND   A131 steel grains are deposited on the top of coarse
            and surrounded by fine martensite. The IPF mappings   304L substrate grains. Compared to the microstructure
            (Figure 10B) further confirmed dendritic crystal formation   of the single-pass track at the top (Figure  10A-C) and
            along the build direction, consisting of columnar and fine-  middle (Figure  10D-F) regions, the grains near the
            equiaxed grains with a weak (101) crystal orientation and a   substrate (Figure 10H) resemble the fine-grained regions
            huge misorientation angle of 5.24° (Figure S4). The average   (Figures  4A; 5D and  E; and 6), and the misorientation
            equivalent grain size was 6.33  µm, with a maximum of   significantly decreased (Figure S6). The average grain size
            83.6 µm due to dendritic growth of the columnar grains.  is approximately 5.45  µm (Figure  10I), slightly smaller
              Figure 10D displays the microstructure of the single-  than that of AB A131 steel (6.8  µm), with a maximum
            pass track in the middle region, featuring coarse columnar   diameter of 31.6  µm. This suggests that laser thermal
            grains and acicular martensite. Compared to the top   cycling promotes submicron-scale grain growth, leading
            region (Figure  10A-C), the columnar grains are more   to a slight increase in the average size. Such effects
            evident (Figure 10E), indicating significant coarsening due   facilitate the formation of alternating fine-  and coarse-
            to  limited  thermal  conduction  and  a  lower  temperature   grain regions during one-pass deposition. Subsequent
            gradient at the center of the melt pool.  This results in   passes remelt the surface with similar thermal gradients
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            a discrepancy in grain size from the center to the edge,   to those near the 304L substrate, promoting the formation
            accompanied by increased crystal misorientation of 6.03°   of fined equiaxed crystals. These repeated thermal cycles
            (Figure S5). The average grain size slightly decreased   contributed to the uniform distribution of heterogeneous
            to 5.93  µm, but the maximum grain size significantly   structures at alternating layers.
            increased to 146.8 µm with a high area ratio (Figure 10F),   To further investigate the heterostructure on
            substantially greater than in AB A131 steel (Figure  6).   anisotropic mechanical performance, an MD model of the
            This suggests that alternating remelting and cyclic thermal   sandwich structure was built, consisting of the fine- and
            effects helped refine the coarse columnar grains.  columnar-grain regions with a similar volume ratio


            Volume 4 Issue 3 (2025)                         10                        doi: 10.36922/MSAM025220038
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