Scandium

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Scandium

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Orbitals and Energies #

Note – these are listed in BINDING ENERGY

 

Sc 2p ≈ 399 eV

Sc 2s ≈ 500 eV

Sc 3s ≈ 54 eV

Sc 3p ≈ 32 eV

Doublet Separations #

Sc 2p = 4.8 eV

Common Overlaps for Sc 2p #

N 1s – Yb 4p – Tb 4s – Ta 4p – Cd 3d – Tl 4d

Auger Energies #

Note – these are listed in KINETIC ENERGY

 

Sc LMM ≈ 1150 eV

Common Binding Energies – Sc 2p #

Species #

B.E. / eV #

Charge Ref #

Reference #

Sc Metal

398.45

Au 4f (83.98 eV)

ScOOH

402.87

C 1s (284.8 eV)

ScBr3

400.8

C 1s (284.8 eV)

ScCl3

401.2

C 1s (284.8 eV)

ScF3

405.3

C 1s (284.8 eV)

Sc2O3

401.6

C 1s (284.8 eV)

Sc2(CO3)3

402.6

C 1s (284.8 eV)

Sc2(CO3)4

403.9

C 1s (284.8 eV)

Sc(NO3)3

403.4

C 1s (284.8 eV)

Theory and Background #

Scandium exhibits more classical behaviour in XPS, compared the the other first row transition metals. With Coster-Kronig transitions energetically unfavourable, and a lack of unpaired valence electrons results in no asymmetric peak broadening, or multiplet splitting – both features of first row TM XPS.

There is, however, significant peak asymmetry for Sc metal, owing to the high degree of electron density around the Fermi energy.

Experimental Advice #

Scandium overlaps significantly with N 1s – and as such, recording the Sc 2s as well as the Sc 2p will allow a secondary check in the event of significant amounts of both elements.

Data Analysis Guidance #

The main oxygen peak for Sc2O3 lies at 529.7 eV.

A hydrated/hydroxide species may lie at 531.8 eV. (1)

Fitting of native oxide overlayers may require use of a suboxide feature at around 400.5 eV.

Reference Datasets #

 

Coming soon

References #

  1. Biesinger, Mark C., et al. “Resolving surface chemical states in XPS analysis of first row transition metals, oxides and hydroxides: Sc, Ti, V, Cu and Zn.” Applied surface science 257.3 (2010): 887-898. Read it online here.
  2. Zimina, Anna, Aline Léon, and Ralph Steininger. “Chemical bonding effects in Sc compounds studied using X-ray absorption and X-ray photoelectron spectroscopies.” Physical Chemistry Chemical Physics 26.3 (2024): 2613-2621. Read it online here.