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Ion Scattering Spectroscopy
Ion scattering spectroscopy (ISS) provides quantitative elemental composition information from the very outermost atomic layer of a surface.
In ISS measurements, a low-energy probe beam of noble gas ions is applied to the sample surface. These ions undergo elastic back-scattering interactions with the outermost surface atoms, during which energy – in the form of momentum – is transferred. The magnitude of momentum transfer is dependent on the elemental species of the sample atom: lighter elements (with closer relative mass to the probe ions) will cause greater reduction in the noble ion’s kinetic energy. The ISS detector measures the amount of back-scattered noble ions with particular kinetic energies, and scans over a range of energy values up to the incident beam energy. By taking the difference between the original and final kinetic energies of the back-scattered ions, the system produces a spectrum of peaks with energy indicative of elemental species, and intensity indicative of quantitative concentration.
- Maximally surface-selective: signal isolated from outermost atomic monolayer
- Highly sensitive, quantitative elemental composition
- No calibration standards required for quantification
- Nondestructive analysis
- Can measure buried interfaces via depth profiling
- Difficult to accurately measure light-element films over heavy-element substrates
- Surfaces must be clean to get good results
- Solid phase
- Must be stable under high vacuum
- Maximum Thickness: 20 mm
- Maximum Lateral Dimensions: 60 mm x 60 mm
Thermo Scientific Nexsa
- Spot Size: 1 mm
- Sensitivity: depends on the noble gas species used for the ion beam
- X-ray Source: monochromated, micro-focused, high-efficiency Al Kα X-ray Anode
Overlay of 3 ISS survey scans of a sputtered Platinum (Pt) film, captured after 3 sputtering segments: at 0 seconds (before sputtering), an oxide layer is present; after 60 seconds of sputtering, the O peak is nearly extinguished, and the Pt signal is very strong; after 90 seconds of sputtering, the O peak is fully eliminated
Overlay of 3 ISS survey scans taken on 3 different film species, showing peak separation for Copper (Cu), Silver (Ag), and Gold (Au)
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