Task-focused Workflow

Calculate Crystallite Size and Microstrain with Williamson-Hall

Review XRD peak broadening with a Williamson-Hall analysis. Inspect the selected peaks and fit before reporting size and strain estimates.

NotyPlot: Scientific Plotting & Peak Analysis XRD williamson hall
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InputSeveral suitable XRD peaks with known wavelength and corrected broadening.
OutputA Williamson-Hall fit with size and strain estimates.

Workflow

  1. Import the XRD pattern and confirm wavelength and instrument-broadening settings.
  2. Detect and fit a set of suitable peaks using a consistent fitting approach.
  3. Select only peaks with defensible fitted widths for Williamson–Hall analysis.
  4. Run the transformation and inspect the included points and fitted line in the Williamson–Hall view.
  5. Review scatter, slope, intercept and warnings; remove a peak only for a defensible fit or data-quality reason.
  6. Report size and microstrain estimates together with the model, selected peaks and fit limitations.

What this workflow helps you do

Separate size-related and strain-related contributions to XRD peak broadening with a Williamson–Hall analysis built from several reviewed fitted peaks. The workflow emphasizes peak eligibility and the transformed linear fit because a numerical intercept and slope are only useful when the selected peaks support the model.

Use this workflow when

  • Estimating crystallite size and microstrain from several diffraction peaks.
  • Comparing broadening behavior across samples using a common XRD model.
  • Checking whether a single-size Scherrer interpretation is masking systematic strain-related broadening.

What you need before you start

  • Several fitted XRD peaks with reliable corrected widths.
  • Known X-ray wavelength and appropriate instrumental-broadening information.
  • Peak selection covering a useful angular range for the Williamson–Hall fit.

Step-by-step workflow

  1. Import the XRD pattern and confirm wavelength and instrument-broadening settings.
  2. Detect and fit a set of suitable peaks using a consistent fitting approach.
  3. Select only peaks with defensible fitted widths for Williamson–Hall analysis.
  4. Run the transformation and inspect the included points and fitted line in the Williamson–Hall view.
  5. Review scatter, slope, intercept and warnings; remove a peak only for a defensible fit or data-quality reason.
  6. Report size and microstrain estimates together with the model, selected peaks and fit limitations.

What to review in the result

  • Enough suitable peaks are included to support a linear trend.
  • No single questionable peak dominates the fitted slope or intercept.
  • Instrument-corrected widths remain physically meaningful.
  • Scatter and fit quality are acknowledged rather than hidden by the final values.

Before you report or export

  • Keep a record of included and excluded peaks.
  • Use the same width definition and correction settings across all peaks.
  • Describe the specific Williamson–Hall model assumption when interpreting size and strain.

Limitations and interpretation

  • Williamson–Hall assumes a simplified relationship between size and strain broadening; real materials may show anisotropy or nonuniform strain that violates it.
  • A small number of peaks or strong scatter can make the fit unstable.
  • Instrumental broadening and peak overlap can bias both the size and microstrain estimates.

Continue your work

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