Arsenic

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Arsenic

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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

Doublet Separations #

As 3d = 0.7 eV

 

As 3p = 4.8 eV

As 2p = 35.8 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

Auger Energies #

Note – these are listed in KINETIC ENERGY

 

As LMM ≈ 1225 eV

Common Binding Energies – As 3d #

Species #

B.E. / eV #

Charge Ref #

Reference #

As (0)

41.5

Au 4f (83.96 eV)

GaAs

40.9

Au 4f (83.96 eV)

As2O3

44.9

C 1s (284.8 eV)

NiAs

41.1

C 1s (284.8 eV)

As2O5

46.2

C 1s (284.8 eV)

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)

The As(3d) and As(2p3/2) regions of an as received GaAs sample. Green = elemental, blue = oxide

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

Reference Datasets #

 

Coming soon

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