1 Introduction

Laser Powder Bed Fusion (LPBF), also known as Selective Laser Melting (SLM), is an additive manufacturing process that is used in industries, such as aerospace, automotive, and medical. In the LPBF process, a metal powder material is applied in thin layers to a substrate plate and then selectively melted using a focused laser beam, resulting in a three-dimensional component. Compared to subtractive processes such as turning and milling, the LPBF process allows greater design freedom without the use of wear tools but also enables the manufacturing of lightweight structures such as lattices. In addition, additive manufacturing can be used to extend the lifespan of certain components by incorporating cooling channel structures into the component [1, 2].

The processing of tool steels with the LPBF process is an active research topic. These steels are characterized primarily by their high hardness and good wear properties and are therefore used primarily in the field of e.g. tool or mould applications [3]. However, only a few tool steels have been qualified for the LPBF process so far. The most common tool steels in LPBF include hot work steels like 1.2709, AISI H11 (1.2343), and AISI H13 (1.2344). Also, high-speed steels with higher carbon content, such as AISI M50 (1.3325) or HS6-3-5‑8 (1.3294) can be processed additively [3,4,5,6].

However, the alloying concepts and the associated microstructures of these steels favor the formation of cracks [3]. For example, cold cracks can form when a manufactured part cools below its solidus temperature. Internal stresses, triggered by the formation of carbides or brittle phases such as martensite, exceed the local material properties and cause cracking [7, 8]. Such cold cracks can be suppressed with the help of a build plate preheating system [9]. In addition to cold cracks, hot cracks can also occur mostly as transcrystalline defects at temperatures between the solidus and liquidus temperature [7]. Hot cracks can be divided into re-melting cracks (RC), solidification cracks (SC), and ductility dip cracks (DDC). RC mostly occur due to stresses during the solidification of low-melting regions in the underlying layers that are reheated when the new layer is melted [10]. SC are formed during solidification shrinkage of low-melting alloying elements at the crystallization front and form at the rounded dendrite tips [8, 11, 12]. DDC is formed by brittle microstructural components, such as martensite or carbides, which are not remelted during exposure. This reduces the ductility of the microstructure, which can lead to stresses [12].

This contribution focuses on the formation of hot cracks in specimens made with LPBF of high-speed steel HS2-2‑2, also known as 1.3294 or ASP®2012, with 0.6 wt.-% carbon content. For this purpose, the influences of laser power (PL), scan speed (vs), layer height (HL), hatch distance (ys), and build plate preheating temperature (BPPT) on the formation of hot cracks are evaluated. Additionally, the density, melt pool geometry, and hot cracks of the produced specimens are measured to further examine the relationship between the processing conditions and the resulting properties.

2 Materials and Methods

Within the scope of this study, the high-speed steel HS2-2‑2 is used. HS2-2‑2 is a cobalt-free high-speed steel that displays high toughness up to a hardness of 58 HRC in cold, warm, and hot applications. Applications for this steel include cold working dies, plastic injection molders and dies for extrusion, forging, and hot forming. The chemical composition of the powder material as specified by the manufacturer Erasteel GmbH is displayed in Table 1 [13].

TABLE 1 Chemical composition of HS2-2‑2 by Erasteel GmbH [13]

All experiments conducted within the scope of this contribution were performed on a laboratory-scale LPBF machine (Aconity Midi) from Aconity3D GmbH, Germany. The machine is equipped with an Ytterbium fiber laser from Rofin-Sinar Laser GmbH, Germany, with a wavelength of 1070 nm and a maximum power output of 400 W. The circular laser spot with an 80 μm diameter (1/e2) in the focal plane has a gaussian intensity distribution. The machine is furthermore equipped with a 3D scan system from Scanlab GmbH, Germany (varioSCAN40 and intelliSCAN20) and a resistive preheating system, that can heat the base plate to 800 °C. All experiments were carried out under an argon inert gas atmosphere with an oxygen content below 200 ppm with approx. 50 mbar overpressure to the ambient atmosphere.

In the experiments, cube-shaped test specimens with a dimension of 10 × 10 × 10 mm3 were produced, using a zig-zag pattern with an alternating hatch rotation of 90° per layer as an exposure strategy. The feed direction of the laser is always turned 45° against the shielding gas flow. The specimens are arranged in a grid on the build plate, and the process parameters are randomly assigned to the individual specimens. For different BPPTs used in the experiments, the preheating system was programmed to a heating ramp of 10 K/min for heat up and cool down after the build job.

The experiments were carried out using BPPTs of Room Temperature (RT), 200 °C, 350 °C, and 500 °C. For the experiments conducted under RT, no BPPT was set. Additionally, the process parameters laser power (PL), scan speed (vs), layer height (HL) and hatch distance (yS) were varied. The overall variations of the different process parameters are shown in detail in Fig. 1.

Fig. 1
figure 1

Variation of the process parameters laser power (PL), scan speed (vs), preheating temperature (BPPT), layer height (HL), and hatch distance (ys)

After manufacturing, the specimens were cut from the substrate plate using electrical discharge machining (EDM) wire cutting and then cut perpendicular to the melt tracks of the topmost layer using a wet cutting machine. The specimens are then ground and polished with 1 µm diamond suspension. The resulting cross-sections were then examined by light optical microscopy (LOM) using the microscope Olympus BX53M from Carl Zeiss Microscopy GmbH. The microscopy images were also used to determine the relative density and the ratio of the measured total crack area to the reference measured area (CAA). Selected cross-sections were etched with 10% aqueous nitric acid to reveal the microstructure and to determine the melt pool dimensions in the topmost layer. The melt pool width (MPW) and the melt pool depth (MPD) were then used to determine the melt pool area (MPA). For this purpose, axisymmetric melt pools were assumed, whose area was approximated with a triangle.

3 Results and Discussion

Figure 2 shows the relative density of all specimens built up with the parameters given in Fig. 1 over the volume energy (Ev). Vertical dashed lines indicate a volume energy range from 40 to 75 J/mm3 and horizontal dashed lines indicate a relative density of 99.50%. The specimens shown in graphs a) to d) were built with HL = 30 µm and with BPPT = RT, 200 °C, 350 °C, and 500 °C. The specimens shown in the graphs e) to g) were built with BPPT = 200 °C and with HL = 30 µm, 40 µm, 50 µm, and 60 µm. Graph b) includes specimens built with ys = 80 µm, 100 µm, and 120 µm. For all other specimens, ys = 100 µm was used.

Fig. 2
figure 2

Relative density over Ev for HL = 30 µm, 40 µm, 50 µm, 60 µm and BPPT = RT, 200 °C, 350 °C, 500 °C

The results shown indicate that relative densities of more than 99.50% can be achieved in a volume energy range from approx. 40 J/mm3 to approx. 75 J/mm3 over all BPPTs, HL and ys. Except for the specimens built with HL = 60 µm, relative densities of more than 99.90% can be achieved in multiple specimens in all experiments. For specimens in a volume energy range from 75 to 175 J/mm3, an increasing scattering of the measured relative densities can be observed. For volume energies below 30 J/mm3 and above 175 J/mm3 no specimens with a relative density above 99.50% could be produced. Specimens built at BPPT = RT show densities of 99.50% for the most part. However, large cold cracks were found in many of these specimens.

Figure 3 shows the evaluation of hot cracks as CAA over the Ev for the same specimens displayed in Fig. 2. The assignment of the specimens to the graphs also corresponds to Fig. 2. Here, vertical dashed lines indicate a volume energy range from 40 to 75 J/mm3 and horizontal dashed lines indicate a CAA of 1%.

Fig. 3
figure 3

CAA over Ev for HL = 30 µm, 40 µm, 50 µm, 60 µm and BPPT = RT, 200 °C, 350 °C, 500 °C

Specimens built at room temperature partly show macroscopic cracks in the form of cold cracks. These cold cracks are not included in the evaluation of the hot cracks and therefore do not influence the CAA value. Specimens built with BPPT = 200 °C and above do not exhibit this kind of cold cracks anymore. With increasing volume energy, the CAA value increases across all experiments. In addition, a greater scattering of the measured values can be observed with increasing volume energy. In a volume energy range of 40 to 75 J/mm3, the smallest average CAA value of 0.28% ± 0.26% can be measured for specimens built with BPPT = 200 °C and HL = 30 µm. The largest average CAA value of 2.52% ± 2.02% occurs for specimens built with BPPT = 200 °C and HL = 40 µm. The smallest overall CAA value with a value of 0.0185% is measured for specimens built with ys = 80 µm, BPPT = 200 °C, and HL = 30 µm. Specimens manufactured at BPPT = 350 °C with HL = 30 µm show the highest total CAA values of up to 5.90%. The reason for the mostly low CAA values in specimens with HL = 50 µm has yet to be determined.

Figure 4 shows the MPD (a) and MPW (b) over Ev for all experiments conducted. The results show that both the width and depth of the melt pools increase with increasing Ev. For specimens manufactured with HL = 30 µm, the average MPD and MPW in an Ev range between 40 and 75 J/mm3 are 110 µm ± 20 µm and 137 µm ± 22 µm respectively.

Fig. 4
figure 4

a MPD over Ev and (b) MPW over Ev for HL = 30 µm, 40 µm, 50 µm, 60 µm and BPPT = RT, 200 °C, 350 °C, 500 °C

Figure 5 shows the overall variation of the resulting MPA over Ev (a) and CAA over MPA (b) for BPPTs from RT to 500 °C and HLs from 30 to 60 µm. In Fig. 5a vertical dashed lines mark an Ev range from 40 to 75 J/mm3, while the horizontal dashed lines mark an MPA range from 0.004 mm2 to 0.012 mm2. In Fig. 5b vertical dashed lines mark an MPA range from 0.004 mm2 to 0.012 mm2, while the horizontal dashed line marks a CAA value of 1%.

Fig. 5
figure 5

a MPA over Ev and (b) CAA over MPA for HL = 30 µm, 40 µm, 50 µm, 60 µm and BPPT = RT, 200 °C, 350 °C, 500 °C

The results displayed in Fig. 5a show an increasing MPA with increasing Ev. In the Ev range of 40 to 75 J/mm3 described above, MPAs of up to 0.03 mm2 are produced across all process parameters. For Ev > 75 J/mm3 a greater scattering of the measured values is observed. MPAs smaller than 0.004 mm2 generally do not occur. Taking the results from Fig. 4 into account, this shows that narrow and shallow melt pools are formed at lower Ev and wider and deeper melt pools are formed at higher Ev. Figure 5b shows that larger MPAs tend to lead to larger CAAs. MPAs up to 0.012 mm2 produce CAA values below 1% across all process parameters with only a few exceptions. In these exceptional cases, large-scale tethering errors with adjacent cracks were found to affect the measured CAA. This boundary partially also applies for MPA greater than 0.012 mm2, but a greater scattering of the measured values is observed here. These results show that the CAA decreases with a smaller MPA and thus narrower and shallower melt pools.

Since the volume energy combines several process parameters (PL, vs, HL, ys), the influences of these parameters are examined individually in more detail in the following. Figure 6 shows the CAA and MPA over ys, BPPT and HL for four different line energies (EL) ascending from left to right within a bar group with EL,1 = 0.2 J/mm, EL,2 = 0.203 J/mm, EL,3 = 0.27 J/mm and EL,4 = 0.3 J/mm.

Fig. 6
figure 6

CAA and MPA over ys, BPPT and HL for EL,1–EL,4

The specimens in Fig. 6a and b were produced with BPPT = 200 °C and HL = 30 µm. For the specimens of Fig. 6c and d, HL = 30 µm and ys = 100 µm were used. The specimens in Fig. 6e and f were produced with BPPT = 200 °C and ys = 100 µm.

Figure 6a, c and e show that the investigated process parameters ys, BPPT, and HL have a separate influence on the CAA value. On average, a decrease in the CAA with increasing ys can be observed. However, for 80 and 100 µm, a larger difference in the CAA values can be observed with increasing EL. At 120 µm, comparatively small CAA values are measured. The preheating temperature (Fig. 6c) is shown to have a significant influence on the CAA value, which is even larger than the influence of the different EL. The highest CAA values are measured at BPPT = 350 °C, whereas the lowest CAA values are measured at BPPT = RT. Similarly, with a variation of HL (Fig. 6e, f), where the highest CAA values are measured at HL = 40 µm while the lowest CAA values are measured at HL = 50 µm.

Figure 6b shows that the hatch distance does not seem to have a significant influence on the MPA, here the difference in EL predominates. In contrast, in Fig. 6d, the MPA tends to increase with increasing BPPT. Figure 6f shows that although the MPA increases with increasing EL, it does not show larger deviations with constant EL over all layer heights.

Figure 7a shows cross-sections of six specimens built at BPPT = 200 °C and an etched segment of the topmost layers of each specimen. The melt pool boundary of individual melt pools is highlighted by a dashed line. The cross-sections shown are parallel to the buildup direction z, as indicated. The first three specimens are fabricated with vs = 740 mm/s and with PL = 150 W, 200 W, and 300 W. The remaining three specimens are fabricated with PL = 200 W and with vs = 500 mm/s, 740 mm/s, and 1000 mm/s.

Fig. 7
figure 7

a Cross-section and melt pool shape of specimens built at BPPT = 200 °C with different laser powers and scan speeds and (b) top view of the topmost layer of a specimen built at BPPT = 200 °C with PL = 300 W and vs = 740 mm/s

For all variations of PL and vs cracks occur within the specimens. As PL is increased, so does the number and the area of the cracks. The same is observed with decreasing scan speed. Therefore, an increase in the number and size of the cracks can be observed with an increasing line energy. However, the morphology of the cracks remains largely the same. All cracks appear at periodic intervals along the x‑axis running parallel to the buildup direction z. As the number increases, cracks increasingly line up in rows. As indicated through the white dashed lines the shape and size of the melt pool also change with line energy. It seems to be irrelevant for the size of the melt pools whether EL is controlled by a change of vs or PL. However, the shape of the melt pools shown seems to change from a drop-like shape for larger EL to an elliptical shape for smaller EL when vs is adjusted at constant PL. When PL is adjusted at constant vs, the drop shape seems to be maintained.

Figure 7b shows the topmost layer of the specimen built with BPPT = 200 °C, PL = 300 W, and vs = 740 mm/s before cutting. It is noticeable that the visible cracks run perpendicular to the melt tracks in the x‑direction. This contradicts the expectation, based on the cross-sections in a), that the hot cracks run parallel to the melt tracks. This could be due to cracks developed in adjacent lower layers continuing at the surface. As can be seen in a), the cracks in the cross-sections seem to run partly across several layers, which supports this assumption.

Figure 8 shows the etched cross-sections of the last layer of four different specimens prepared with parameters that yield ascending line energies corresponding to the ones described above. The melt pool boundary containing a crack is highlighted by a dashed line for each individual specimen. The melt pools vary in width and depth as well as in the melt pool shape, which ranges from elliptical to drop-shaped. All highlighted melt pools are intersected by a crack in the center. The paths of the cracks vary. In Fig. 8a, the crack starts in the center of the melt pool and runs into the adjacent layers below it. In Fig. 8b, the crack divides the melt pool vertically and stops at the melt pool boundary. The crack therefore does not connect to other visible cracks in the adjacent layer below that connects to the same melt pool boundary. In Fig. 8c,d, the crack starts in the center of the melt pool and ends at the boundary of the melt pool.

Fig. 8
figure 8

Etched cross-section of four specimen EL,1, EL,2, EL,3 and EL,4 built with BPPT = 200 °C with cracks running through individual melt pools

Figure 9 shows detailed LOM pictures of two melt pools from specimens with EL = 0.47 J/mm and EL = 0.17 J/mm respectively.

Fig. 9
figure 9

Melt pools of specimens built with BPPT = 200 °C and ys = 100 µm; a with EL = 0.47 J/mm and average MPA = 0.056 mm2; b detail of the crack from a and c with EL = 0.17 J/mm and average MPA = 0.006 mm2

For the specimen from Fig. 9a, an average MPA of 0.056 mm2 is measured. The arrows indicate the orthogonal growth direction of the dendrites from the melt pool edge. Dendrites along the steep melt pool flank are almost parallel oriented to each other and grow toward the center of the melt pool. A crack has formed between the solidification fronts that have been created (Fig. 9b, Sect. 1). This upper part of the crack is orthogonal to the dendrites and has rather irregular crack edges, leading to the assumption that it might be a solidification crack. The lower part of the crack shown in Sect. 2, on the other hand, has sharp crack edges, suggesting that it could be a cold crack initiated from the hot crack above. The underlying mechanism here is assumed to be the stresses that arise during the solidification of the dendrites due to shrinkage against the direction of solidification. The melt pool shown in Fig. 9c, with an average MPA of 0.006 mm2 also shows dendrites growing orthogonal to the melt pool edge. In contrast to a), the dendrites meet here at various angles, which can be attributed to the absence of steep melt pool edges as can be observed for a).

4 Conclusion

In this contribution, the occurrence of hot cracks during the processing of HS2-2‑2 by LPBF was investigated with a variation of the process parameters laser power, scan speed, hatch distance, layer height, and build plate preheating temperature. Two different types of cracks were found in the cross-sections of the manufactured specimens. Large cracks have occurred isolated without preferential direction. These are identified as cold cracks based on their course and shape. In addition, periodic microcracks with a clear preferred direction along the buildup direction have been detected in almost all specimens. The melt pool analysis has shown that these cracks are preferentially found in the center of individual melt pools, hence the cracks are identified as hot cracks or specifically as solidification cracks.

Density evaluations show that specimens with a relative density of 99.5% can be produced at a volume energy range of 40 to 75 J/mm3. In addition, cold cracks can be prevented with a preheating temperature of 200 °C or more. Furthermore, it can be shown that the shape and size of the melt pools are dependent on the volume energy; larger volume energies therefore tend to produce larger melt pool widths and depths.

The analysis of the influences of the process parameters laser power, scan speed, hatch distance, layer height, and preheating temperature on crack formation has shown that the laser power and scan speed, hence the line energy, have the largest influence on the melt pool shape and size as well as the crack formation. Smaller line energies lead to decreasing melt pool widths and depths and thus smaller melt pool areas. This is due to the fact that higher energy inputs trigger deep-welding effects, while heat conduction welding effects increasingly come into play at lower energy inputs. These heat conduction welding effects produce rather elliptical melt pool shapes instead of drop-like melt pool shapes as is the case for the deep welding effects. The steep flanks of the drop-shaped melt pools, which run almost orthogonally to the build platform, favor the growth of dendrites from the side walls to the center axis of the melt pools, which in turn favors the formation of hot cracks in the form of solidification cracks along the center axis of the melt pools. In the elliptical melt pools, these steep melt pool flanks do not occur which leads to a growth of the dendrites under various angles with a decreased formation of hot cracks. From this, it can be concluded that hot crack formation can be controlled primarily by the shape of the melt pools. It was shown that a change of the melt pool shape from a drop shape to an elliptical shape can rather be achieved by adjusting the scan speed.

Furthermore, it is shown that the formation of hot cracks can already be reduced without the use of a preheating system but peaks at a build plate preheating temperature of 350 °C. For the different layer heights, no correlations could be derived. However, for a layer height of 50 µm, higher densities and lower CAA values are measured throughout.

The combined influences of the investigated process parameters on the melt pool shapes and sizes and thus the formation of hot cracks remain to be investigated. A more in-depth classification of the observed cracks by examining the microstructure also remains to be done.