Steel Hardening Processes - An Overview
Steel is a versatile material in industry and is particularly popular for its robustness. However, this robustness is not a fundamental property of steel, but in many cases the result of purposeful thermal processes. In this article, we introduce the processes of steel hardening, provide an overview of hardening methods, and list common errors and problems.
How is steel hardened?
Steel is defined in the standard DIN EN 10020 as an alloy of iron with a carbon content of max. 2.06%. In addition to other alloying elements, the carbon content has a direct influence on whether or not a steel can be hardened. Structural steels with a carbon content below 0.2% can generally not be hardened. With a carbon content of approx. 0.25% to 0.4%, hardening by additional carbon input is possible (case-hardened steels). Starting at 0.4% carbon, steels can be hardened by common hardening methods. If the carbon content increases to more than 2.06%, the transition from steel to so-called cast iron begins.
The iron-carbon diagram is useful for making the effect of the carbon content on the material properties of steel a little clearer. The iron-carbon diagram shows the transformation of the individual phases (microstructure composition), provided that the steel always has sufficient time for the respective phase transformation. The microstructural change at different cooling rates cannot be shown. For this purpose, a separate time-temperature transformation diagram is created for each alloy.
The Iron-Carbon Diagram
In the iron-carbon diagram shown here, the range of the liquidus and solidus lines is only shown in simplified form. Above the liquidus line, the mixture is liquid; between the liquidus and solidus lines, the alloy has a mushy consistency. Below the solidus line, the alloy is solidified, but is present as a different phase depending on the carbon content with different intercalation mixed crystals depending on the respective phase.