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Laser Powder Bed Fusion

SLMDMLSDMLMLaserCUSINGPBF-LB/M

Ytterbium fibre laser, typically 200–1000 W, wavelength 1060–1080 nm (near-infrared). Multi-laser configurations: 2, 4, 8, or 12 lasers in parallel.

Layer thickness
20–100 µm
Tolerance
±0.05–0.3 mm
Surface Ra
5–25 µm
Build rate
5–80 cm³/h
Relative density
99–99.9 %
Min wall
0.2 mm (typ. 0.4 mm)
Min feature
0.3 mm (typ. 0.5 mm)
Supports required
Yes

How it works

A fine powder (typical D50 10–45 µm) is spread in a thin layer (~20–100 µm) across a build platform by a recoater blade or roller. A focused laser beam traces the cross-section of each layer, selectively melting the powder to form a dense melt pool that fuses to the previous layer upon solidification. Unmelted powder supports the part and is recovered for reuse. The process occurs in a sealed chamber purged with argon or nitrogen to an oxygen level below 500–1000 ppm. Repeating layer-by-layer produces a three-dimensional near-net-shape component with typically >99.5% relative density. Residual stress builds up due to rapid thermal gradients — most metals require stress relief after build.

Parameter envelopes (6 material–machine combinations)

Ti-6Al-4V Grade 5(EOS M 290)argon

Power

200340 W (typ. 280 W)

Scan speed

8001800 mm/s

Layer thickness

3060 µm

Hatch spacing

100140 µm

Max O₂

500 ppm

Preheat

35 °C

VED optimal

5570 J/mm³

EOS standard parameter set for Ti-6Al-4V on M 290 at 30 µm layer. Preheat to 35°C minimises first-layer thermal shock. VED above 80 J/mm³ risks keyhole porosity; below 50 J/mm³ risks LOF defects.

316L Stainless Steel(EOS M 290)nitrogen

Power

180370 W (typ. 275 W)

Scan speed

7001400 mm/s

Layer thickness

2050 µm

Hatch spacing

90130 µm

Max O₂

1000 ppm

Preheat

80 °C

VED optimal

6590 J/mm³

Nitrogen atmosphere is acceptable and cheaper than argon for 316L. Preheat to 80°C reduces residual stress and improves dimensional accuracy on complex geometries.

AlSi10Mg(EOS M 290)nitrogen

Power

250400 W (typ. 370 W)

Scan speed

13002200 mm/s

Layer thickness

3060 µm

Hatch spacing

130190 µm

Max O₂

1000 ppm

Preheat

150 °C

VED optimal

5065 J/mm³

AlSi10Mg requires 150–200°C preheat to prevent thermal cracking. Al reflects ~8% of 1070 nm laser — higher power required vs steel. Hot tearing risk above 200°C preheat with some alloys.

Inconel 718(EOS M 290)argon

Power

250400 W (typ. 285 W)

Scan speed

8001400 mm/s

Layer thickness

2060 µm

Hatch spacing

90130 µm

Max O₂

500 ppm

Preheat

80 °C

VED optimal

6085 J/mm³

IN718 is susceptible to hot cracking at high VED. Columnar grain texture and Laves phase formation are as-built. All structural applications require SA+DA heat treatment.

CoCrMo(EOS M 290)argon

Power

150300 W (typ. 200 W)

Scan speed

7001300 mm/s

Layer thickness

2040 µm

Hatch spacing

80120 µm

Max O₂

500 ppm

Preheat

80 °C

VED optimal

80110 J/mm³

CoCrMo has high laser absorptivity (~45% at 1070 nm). High hardness (as-built ~35 HRC) makes support removal difficult — minimise support contacts or use breakaway pedestals.

Maraging Steel MS1 (18Ni-300)(EOS M 290)argon

Power

150370 W (typ. 200 W)

Scan speed

7001400 mm/s

Layer thickness

2050 µm

Hatch spacing

80120 µm

Max O₂

500 ppm

Preheat

35 °C

VED optimal

6080 J/mm³

Maraging MS1 as-built is ductile soft martensite (~33 HRC). Machine in soft state, then age at 480°C/6h for 54 HRC. Near-zero dimensional change on ageing (<0.1% linear). No quench required.

Defect modes (6)

Keyhole Porosity

Cause

Excessive Volumetric Energy Density (VED) above the keyhole threshold, typically >80–100 J/mm³ for most alloys. The laser creates a deep, narrow vapour-filled cavity (keyhole) that collapses and traps gas.

Indicator

Spherical pores (diameter 20–200 µm) visible in cross-section micrographs or X-ray CT. Located within scan tracks, not at layer interfaces. Often associated with spatter ejection during build.

Prevention

Reduce laser power or increase scan speed to lower VED. Avoid high-power, low-speed parameter combinations. Characterise keyhole threshold using single-track experiments or VED parameter maps.

Detection

  • X-ray CT
  • Archimedes density measurement
  • metallographic cross-section

Lack-of-Fusion (LOF) Porosity

Cause

Insufficient Volumetric Energy Density: laser does not fully melt the current powder layer or fails to re-melt and bond to the previous layer. Causes: low power, high speed, excess layer thickness, excessive hatch spacing, or degraded powder flowability.

Indicator

Irregular, elongated pores (typically 50–500 µm, aspect ratio >2) often containing unmelted powder particles. Located at layer interfaces or between scan tracks. Catastrophic effect on fatigue life.

Prevention

Maintain VED within validated process window. Use layer thickness ≤particle D90. Ensure powder is dry and within specified refresh ratio. Monitor recoater deposition quality (in-process imaging if available).

Detection

  • X-ray CT
  • metallographic cross-section
  • HIP (remediation, not detection)

Residual Stress and Distortion

Cause

Steep thermal gradients (~10⁶ K/m) from the highly localised laser energy input create differential thermal contraction stresses during cooling. The build plate and support structures constrain the part, building up tensile stress in the top layers and compressive stress in the bottom.

Indicator

Part warps or distorts when removed from build plate. Scan tracks visible as bands of different microstructure in etched cross-sections. Stress relief cracking in susceptible alloys (some IN718, some high-carbon steels).

Prevention

Apply stress relief or HIP post-processing. Use chessboard or island scan strategy to reduce long scan track lengths. Preheat build plate (>80°C for steels, 150°C for aluminium). Simulate residual stress with process simulation software before build.

Detection

  • Neutron diffraction (bulk)
  • X-ray diffraction (surface)
  • strain gauges
  • coordinate measuring machine (CMM) before/after wire-EDM release

Columnar Grain Texture and Anisotropy

Cause

Directional heat extraction along the build direction (Z-axis) during rapid solidification promotes epitaxial grain growth producing <100> textured columnar grains aligned with the Z-axis. This is intrinsic to LPBF physics, not a defect in the traditional sense, but causes mechanical anisotropy: Z-direction properties are typically 5–15% lower than XY for metals.

Indicator

Columnar grain structure visible in EBSD or optical metallography. Mechanical testing shows directional dependence (XY stronger than Z in tensile, opposite in compression in some alloys).

Prevention

Cannot be fully eliminated without HIP or heat treatment. Can be mitigated by: high preheat (>150°C), post-process HIP, or process optimisation for fine equiaxed grains. Grain refiners (Sc, Zr additions to Al alloys) can promote equiaxed solidification.

Detection

  • EBSD
  • optical metallography
  • dual-axis mechanical testing (XY vs Z specimens)

Surface Roughness and Staircase Effect

Cause

Layer-by-layer construction creates staircase steps on inclined surfaces. Down-facing surfaces (overhangs) are rougher (Ra 20–60 µm) than up-facing (Ra 5–15 µm) due to partial particle attachment. Spatter particles adhere to near-vertical walls.

Indicator

Ra > 15 µm on inclined surfaces. Visual staircase pattern at low-angle slopes (<45° from horizontal). Unmelted powder particles embedded in down-skin surfaces.

Prevention

Design with minimum 45° overhang angles. Use contour scan parameters optimised for surface quality (lower power, multiple contour passes). Post-process: abrasive flow machining, electrochemical polishing, shot peening, or CNC machining.

Detection

  • Contact profilometer (Ra per ISO 4288)
  • non-contact white light interferometry (Sa per ISO 25178)

Hot Cracking / Liquation Cracking

Cause

Found primarily in crack-susceptible alloys (CM 247LC, CMSX-4, some Al alloys). Low solidification range alloys with wide mushy zones, or alloys with low-melting grain boundary phases, crack during cooling due to thermal stress exceeding the local hot-strength.

Indicator

Intergranular cracks, typically located at prior austenite grain boundaries or near Laves phase regions (IN718). Often branching and irregular. Visible in etched optical or SEM micrographs.

Prevention

Increase preheat temperature (≥500°C for crack-susceptible Ni superalloys via EBM, which has lower residual stress). Apply HIP to close cracks after build. Select crack-resistant alloy compositions (e.g., Alloy 718C vs. standard 718). Use EBM instead of LPBF for problematic alloys.

Detection

  • Fluorescent penetrant inspection (FPI/FPI)
  • X-ray CT
  • metallographic cross-section

Compatible materials

Governing standards

Related calculators

Last reviewed: 2026-05-04 · v1 · Sources: debroy-2018-review, king-2015-lpbf-overview, eos-ti64-2023, renishaw-316l-2023