
Arsenic #
Orbitals and Energies #
Note – these are listed in BINDING ENERGY
As 3d ≈ 41 eV
As 3p ≈ 141 eV
As 3s ≈ 204 eV
As 4d ≈ 3 eV
Common Overlaps for As 3d #
V 3p – Hf 4f – Ce 5s – Pr 5s – Sr 4s – Pm 5s – Nd 5s – Sm 5s – At 5d – Te 4d – At 5d – Th 6p – Cr 3p – Ru 4p – Ca 3s
Theory and Background #
Arsenic is primarily analysed using the As(3d) region, which can overlap with the Ta(5p1/2) signal. Generally observed as an oxide or in GaAs, the As(3d) region has a spin-orbit splitting of 0.7 eV, with an intensity ratio of 0.7, as opposed to the expected 0.67.
Recording the As(2p3/2) region is useful also and demonstrates oxide thickness as a function of kinetic energy (see below)
Experimental Advice #
It has been reported that As2O3 sublimes in vacuum [1], whereas As5+ may under go some degredation by XPS analysis to yield As3+, so rapid analysis and/or summation of multi-point analysis may be required.
The As LMM Auger peaks when recorded with a Al source encompass a wide energy range (500 – 250 eV) and therefore overlap with many other photoemission lines, so care should be taken in analysis.
Data Analysis Guidance #
N/A
References #
1. Arsenic entry at Thermo Scientific XPS Periodic Table
2. Arsenic entry at www.xpsfitting.com
3. Measured at HarwellXPS on Thermo Scientific K-Alpha+
4. Measured at HarwellXPS on Kratos Axis Ultra DLD system
5. H.W. Nesbitt and M. Reinke, American Mineralogist, 84 (1999) 629. Read online
