Practical XRD with Confidence

3: XRD for Thin Films: Choosing the Right Measurement for Structure, Strain, and Thickness

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This is a written summary of a live webinar presented on June 3, 2026. The recording and resources are available on the recording page.

Presented by:

Keisuke Saito, PhD

Director of Application Science

Rigaku

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Webinar summary

In this webinar, the third in the series Practical XRD with Confidence, Keisuke discusses how thin-film X-ray diffraction requires different measurement choices depending on whether the film is polycrystalline, textured, or epitaxial. A key challenge is preferred orientation. In a powder sample, crystallites are randomly oriented, so a conventional scan can capture many diffraction peaks needed for phase identification. In a thin film, crystallites often align in specific directions because of epitaxial growth on a single-crystal substrate or because low-surface-energy planes tend to align parallel to the surface during deposition. As a result, only certain reflections may appear, making phase identification more difficult.

For polycrystalline thin films, the first recommended measurement is a symmetric 2θ/θ scan. This scan is similar to a powder diffraction scan, but thin-film measurements typically use parallel-beam optics, such as an X-ray mirror, to control the incident beam. In this geometry, the scattering vector is perpendicular to the sample surface, so the scan mainly probes lattice spacings, phase information, and preferred orientation in the out-of-plane direction. The major drawback is penetration depth: X-rays can penetrate deeply, so signals from the substrate or thicker underlying layers can dominate and obscure the signal from a very thin surface layer.

Grazing-incidence methods are used to make XRD more surface sensitive. In an in-plane XRD scan, the X-ray beam strikes the sample at a shallow incident angle, often below one degree, while the detector scans parallel to the sample surface. This makes the scattering vector nearly parallel to the film surface, allowing analysis of in-plane lattice spacings, phase information, and preferred orientation. Changing the incident angle can provide depth-dependent information because it changes how deeply the X-rays penetrate.

Grazing-incidence diffraction, or GID/GIXRD, is another surface-sensitive option. In this approach, the incident angle remains shallow while the detector scans out of plane. It can be performed with a parallel-slit analyzer or with faster one-dimensional detector methods. However, the scattering vector is tilted, and that tilt changes with 2θ, which complicates interpretation when the film has strong preferred orientation. For non-textured thin films, both in-plane XRD and GID can be useful; for textured or oriented films, in-plane XRD is preferred.

A thin-film iron oxide example illustrates the need to choose scan geometry carefully. The surface iron oxide layer was only 5 nm thick, while the underlying copper oxide layer was much thicker. A symmetric 2θ/θ scan was dominated by copper oxide peaks and substrate-related features, although broad peaks from the iron oxide were also visible. Peak widths were used with the Scherrer equation to estimate crystallite size. Copper oxide peaks corresponded to crystallites of about 11 nm, while iron oxide peaks corresponded to about 5 nm crystallites. A sharp feature near 33° was attributed not to a normal silicon 002 reflection, which is forbidden, but to multiple diffraction from the silicon substrate.

Surface-sensitive measurements clarified the iron oxide phase information. By calculating penetration depth near the critical angle for total reflection, the incident angle could be selected to limit penetration to only a few nanometers. An in-plane scan at the critical angle greatly reduced the copper oxide signal and emphasized the iron oxide layer. Magnetite and maghemite were difficult to distinguish because their diffraction patterns are similar in thin-film form, and wüstite could not be confirmed confidently because of peak overlap. However, beta iron oxide was detected in the surface-sensitive scan even though it was not observed in the out-of-plane scan. GID scans at different incident angles showed that higher incident angles penetrated deeper and produced stronger copper oxide peaks, while shallower angles emphasized broad iron oxide peaks.

Instrumental broadening must be considered when crystallite size is estimated from peak width. The measured full width at half maximum contains contributions from the sample and the instrument. Instrument broadening can be determined by measuring a standard reference material, such as silicon, lanthanum hexaboride, or another standard powder, using the same configuration. The corrected peak broadening should be converted from degrees to radians before being used in the Scherrer equation. For thin films, a shape factor of 1.0 is more appropriate than the common powder value of 0.9 because film crystallites are often oriented and not spherical.

Detector resolution is only one contributor to the final diffraction peak width. A detector pixel size of about 0.02° does not automatically mean that peaks separated by 0.02° can be confidently resolved. The observed profile is a convolution of contributions from the X-ray source, optics, slits, sample, and detector. If the incident beam divergence or sample broadening is larger than the detector contribution, the detector pixel resolution alone will not determine peak separability.

High-resolution XRD is mainly used for epitaxial thin films. In this context, the incident angle is usually described as omega rather than theta, because omega may differ from half of 2θ. High-resolution measurements require monochromating the X-ray beam, often down to Cu Kα1, using two-bounce or four-bounce germanium monochromators. Two-bounce monochromators provide higher intensity but more dispersion, while four-bounce monochromators provide more stable resolution over a wider angular range but lower intensity. Analyzer crystals on the receiving side can provide very high 2θ resolution, but they reduce intensity and are most useful when the sample has significant mosaicity.

Several high-resolution scan types provide complementary information. A symmetric 2θ/ω scan probes the out-of-plane lattice parameter and can show thickness fringes or satellite peaks, which can be used to calculate film thickness. An omega scan, or rocking curve, probes mosaicity caused by deviations in crystal orientation, often related to dislocations from lattice mismatch. Reciprocal space mapping combines angular scans to map intensity around reciprocal lattice points, allowing determination of both in-plane and out-of-plane lattice parameters, strain, relaxation, symmetry, and domain structure.

A perovskite thin-film example demonstrates how high-resolution measurements reveal structure. A 45 nm L5BO film on an LSAT substrate was examined using 00L scans and reciprocal space maps. The 00L scan showed layer peaks and clear thickness fringes. The out-of-plane lattice mismatch was calculated from the layer/substrate peak separation as about 0.471%, and the layer lattice parameter was about 0.387 nm. The film thickness calculated from fringe spacing was about 44.2 nm, close to the expected 45 nm. Higher-angle reflections provided better separation between closely spaced substrate and film peaks.

Reciprocal space maps provided additional structural information that could not be obtained from a simple out-of-plane scan. Mapping around a tilted reflection showed multiple layer peaks, indicating multiple domain orientations. The analysis showed a monoclinic structure with an in-plane lattice parameter of about 0.387 nm, a slightly elongated c-axis, and a beta angle about 0.5° away from 90°. Four domains were identified, separated by 90° rotations in the in-plane direction.

Rocking-curve information can be extracted from reciprocal space maps. Around a surface-normal reflection such as 004, the rocking-curve direction is nearly parallel to the QX direction over a small region. Extracting intensity along QX and converting ΔQX/QZ to angular width gave a rocking-curve width of about 0.02°. Separate rocking-curve measurements confirmed this value when a sufficiently narrow receiving slit was used. A wide receiving slit mixes broadening from QX and QZ; because QZ broadening is strongly affected by finite film thickness, a wide slit can make the measurement reflect thickness-related broadening rather than true mosaicity.

Frequently asked questions

Powders usually contain randomly oriented crystallites, so many lattice planes satisfy diffraction conditions during a standard scan. Thin films often have preferred orientation. For example, an FCC film such as copper on glass may align its 111 planes parallel to the surface, causing mainly 111 and higher-order reflections to appear. With only one or two visible peaks, phase identification becomes much more difficult.

A symmetric 2θ/θ scan should be performed first. It gives out-of-plane phase and orientation information and can reveal substrate, layer, and film peaks. Even though it may not be very sensitive to very thin surface layers because of deep X-ray penetration, it provides an important starting point before using in-plane or grazing-incidence methods.

In-plane XRD should be used when the film has preferred orientation or texture and surface-sensitive information is needed. GID/GIXRD is useful for non-textured films, but its scattering vector is tilted and the tilt varies with 2θ, which makes analysis difficult for strongly oriented films. For textured films, in-plane XRD is the better grazing-incidence option.

The incident angle can be set near or below the critical angle for total reflection. At these very shallow angles, penetration depth can be limited to only a few nanometers, depending on the material and X-ray energy. In the iron oxide example, using an incident angle around the calculated critical angle reduced the contribution from the underlying copper oxide layer and made the 5 nm iron oxide layer easier to analyze.

Crystallite size can be estimated using the Scherrer equation, where the peak broadening is related to crystallite size. Broad peaks correspond to smaller crystallites, while sharper peaks correspond to larger crystallites. Instrumental broadening must be subtracted from the measured peak width, and the corrected width must be converted to radians. For thin films, a shape factor of 1.0 is preferred because the crystallites are often oriented and not spherical.

Instrumental broadening is determined by measuring a standard material with the same instrument configuration used for the sample. Suitable standards include reference powders such as silicon or lanthanum hexaboride. The measured full width at half maximum from the standard provides the instrumental contribution, which is then used to correct the sample peak width.

Reciprocal space mapping provides both in-plane and out-of-plane lattice information. It can be used to evaluate lattice mismatch, strain, relaxation, crystal symmetry, and domain structure. It can also reveal whether a film has multiple domain orientations. In addition, rocking-curve information can be extracted from reciprocal space maps, reducing the need for a separate rocking-curve measurement in some cases.

A wide receiving slit can mix broadening from both QX and QZ directions. In thin films, QZ broadening can arise from finite film thickness, so a wide slit may cause the rocking curve to reflect thickness effects rather than true mosaicity. A narrower receiving slit reduces this mixing and provides a better measurement of mosaic spread, although at the cost of lower intensity.

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