The XRD patterns of the five steels indicated that the 0.3 C, 0.6 C, 0.8 C, and 1.1 C steels had a fully austenitic structure with no carbide precipitate, and the 0 C steel had a mechanical-grinding-induced ε-martensite in an austenite matrix. The increase in the lattice parameters of the 0.6 C, 0.8 C, and 1.1 C steels up to 0.78% over that of the 0.3 C steel calculated from the γ(111) peaks suggested that the added carbon was presented as interstitial carbon in the steels. Dot-like MnO and Mn-S-O inclusions with a diameter of less than 10 μm were evenly dispersed in the five steels.
The 0.6 C, 0.8 C, and 1.1 C steels were passivated during the anodic polarization in 0.1 M Na2SO4 solution at pH 12.0, whereas the 0 C and 0.3 C steels actively dissolved. The anodic polarization measurements of the 0.3 C, 0.6 C, 0.8 C, and 1.1 C steels in 0.05 M Na2B4O7-NaOH buffer solution at pH 10.0 with 0.1 M Na2SO4 revealed that the dissolution current density of the steels decreased with higher amounts of interstitial carbon. The dissolution current density at 0.3 V vs. Ag/AgCl (3.33 M KCl) of the 1.1 C steel was reduced to about 1 × 10-2 A m-2, which was one hundredth that of the 0.3 C steel. A new finding demonstrated here is that a higher interstitial carbon content in the Fe-33Mn-C steels resulted in a stronger inhibition in the dissolution current density of the steels, resulting in an improvement in the corrosion resistance of the steels.
The dissolution current density of the steels was not inhibited by CO32- ions, which is the expected dissolution product of the interstitial carbon, during the anodic polarization in Na2CO3-NaHCO3 buffer solution (0.1 M CO32-) at pH 10.0 with 0.1 M Na2SO4. It was confirmed that the decrease in the dissolution current density of the steels as a function of the interstitial carbon content measured in 0.05 M Na2B4O7-NaOH buffer solution at pH 10.0 with 0.1 M Na2SO4 was not the effect of the formation of CO32- ions in the solution. The XPS analysis of the 1.1 C steel detected the chemical shifts approximately 0.1 eV higher in the Fe 2p3/2 electron binding energy and approximately 0.2 eV higher in the Mn 2p3/2 electron binding energy compared with the peak positions of the Fe 2p3/2 and Mn 2p3/2 spectra measured for the 0 C steel. This can likely be attributed to the partial chemical bonding of interstitial carbon to iron and manganese, respectively.
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