Chromium

Doublet Separations

  • Cr 2p: 9.3 eV

The Energies Listed are Binding Energies!

 

  • Cr 2s: 695 eV
  • Cr 2p: 575 eV
  • Cr 3s: 74 eV
  • Cr 3p: 43 eV
  • Cr 3d: 2 eV
Cr2O3 Survey Scan with Peak Markers for Cr Emissions

The Energies Listed are Binding Energies!

Cr is primarily analysed via the 2p orbital

  • Cu LMM (Al source) (566 eV)
  • Ta 4s (566 eV)
  • Rn 4d (567 eV)
  • Ag 3p (571 eV)
  • Hg 4p (571 eV)
  • Te 3d (572 eV)
  • Fr 4d (577 eV)
  • Ir 4p (577 eV)
  • Ru 3s (575 eV)
  • W 4s (595 eV)
Cr2O3 Peaks and Overlapping Peak Markers

Energies listed are Kinetic Energies!

Note – Cr LMM may overlap with O KLL

Cr LMM: ~ 525 eV

Chromium Oxide LMM Auger – Note potential overlap with O KLL

 

 

 

The Energies Listed are Binding Energies!

Species Binding energy / eV Charge Ref Ref
Cr(0) 574.4 Au 4f (84 eV) 1
Cr2O3 576.7 Au 4f (84 eV) 1
Common Chromium Binding Energies

Chromium in particular oxidation states (most notably Cr(III) compounds, due to unpaired electrons) exhibits multiplet splitting. The 2p region exhibits broadening and asymmetry in a number of oxides, while the 3s region splits into two peaks in a manner indistinguishable when above or below the Curie temperature,[2] indicating that the ferromagnetic spin ordering does not influence this splitting. Cr(VI) is diamagnetic and therefore does not exhibit multiplet splitting. CrO2 is sometimes considered as a single pair of asymmetric peaks, due to being a conductive oxide[3] – however given the breadth of the peaks, and the paramagnetic [Ar]3d2 configuration of Cr(IV) it is considered possible to be due to multiplet splitting rather than a asymmetric shake-up processes.[4]

Chromium (VI) is known to photoreduce to tetra- and trivalent species under X-ray illumination.[5] This photoreduction can be greatly accelerated by certain charge neutralisation techniques – such as a dual neutraliser, and as such, care should be taken in selecting a neutralisation mode to minimise rapid sample damage.[6]

Fitting of Cr(III), much like any species with significant multiplet structure, can be a time-consuming task. Models developed from first-principles and standards can go a long way to help,[7] and recording your own data standards can help too.

 

Not available

  1. Salvi, Anna M., et al. “Peak fitting of the chromium 2p XPS spectrum.” Applied surface science 90.3 (1995): 333-341. Read it online here.
  2. Ikemoto, Isao, et al. “X-ray photoelectron spectroscopic studies of CrO2 and some related chromium compounds.” Journal of Solid State Chemistry 17.4 (1976): 425-430. Read it online here.
  3. Bullen, Heather A., and Simon J. Garrett. “CrO2 by XPS: comparison of CrO2 powder to CrO2 films on TiO2 (110) single crystal surfaces.” Surface Science Spectra 8.3 (2001): 225-233. Read it online here.
  4. Biesinger, Mark C., et al. “Resolving surface chemical states in XPS analysis of first row transition metals, oxides and hydroxides: Cr, Mn, Fe, Co and Ni.” Applied Surface Science 257.7 (2011): 2717-2730. Read it online here.
  5. Halada, Gary P., and Clive R. Clayton. “Photoreduction of hexavalent chromium during X‐ray photoelectron spectroscopy analysis of electrochemical and thermal films.” Journal of the Electrochemical Society 138.10 (1991): 2921. Read it online here.
  6. Edwards, Lee, Paul Mack, and David J. Morgan. “Recent advances in dual mode charge compensation for XPS analysis.” Surface and Interface Analysis 51.9 (2019): 925-933. Read it online here.
  7. Biesinger, M. C., et al. “X‐ray photoelectron spectroscopy studies of chromium compounds.” Surface and interface analysis: an international journal devoted to the development and application of techniques for the analysis of surfaces, interfaces and thin films 36.12 (2004): 1550-1563. Read it online here.