Confused by XPS Peaks? Here’s How to Identify Them Step-by-Step!

Confused by XPS Peaks? Here’s How to Identify Them Step-by-Step!

Understanding XPS Spectra: Key Parameters and Characteristics

Overview of XPS Spectra

  • The number of peaks in XPS spectra is influenced by three main parameters: the chemical environment, the physical and chemical state of the sample, and instrumental contributions.
  • A standard XP spectrum from lead illustrates that heavy elements can absorb a large number of photoelectron peaks, which are crucial for analysis.

Identifying Photoelectron Peaks

  • Photoelectron peaks (also known as Shar peaks) can be identified by their sharpness; they indicate emissions from photoelectrons. In contrast, OJ peaks lack this sharpness.
  • Intense and narrow peaks in XP spectra signify photoelectron emissions, which result from convolution involving factors like the width of X-ray interactions and electron lifetime.

Characteristics of Photoelectron Peaks

  • Photoelectron peaks originate from a very thin region (approximately 10 nm) where electrons do not undergo elastic collisions, ensuring maximum kinetic energy reaches the detector. This results in clear photoelectron signals.
  • Less intense peaks at higher binding energies tend to be wider compared to those at lower binding energies; this distinction helps identify insulating materials versus conductors during analysis. Insulating materials typically show wider peaks than conductors.
Video description

How to identify Photoelectron Peaks in XPS spectra? Several types of peaks can be observed in XPS spectra. The chemical environment and other physical and chemical state of the sample can increase/decrease the peaks in XPS spectra. Also the instrumental contribution should be considered. 1- Photoelectron Peaks 2- Auger Peaks 3- X-rays Satellite Peaks 4- X-rays Ghost Peaks 5- Shake-Up Peaks 6- Shake- off peaks 7- Multiplet splitting 8- Energy Loss Lines 9- Valence Lines and Bands Let's discuss Photoelectron Peaks Photoelectron peaks are also called Sharp Peaks and these are the most intense and typically the narrowest peaks observed in the XPS spectra. Peak width is basically a convolution of the width of the x-ray line, the lifetime of the "hole" resulting from the photoionization process, and of course the instrumental contribution. These peaks are due to the photoelectrons generated within the first few atomic layers ~1nm to 10 nm (elastically scattered). Less intense peaks at higher BE are usually wider approximately 1-4 eV than the peaks at lower BE. Moreover, the peaks of insulating materials are wider than the peaks of conductors. Please subscribe to my channel and share it. Thank you so much