Beryllium

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Beryllium

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Orbitals and Energies #

Note – these are listed in BINDING ENERGY

 

Be 1s ≈ 113 eV

 

Doublet Separations #

No non-S orbitals

Common Overlaps for Be 1s #

Ga 3p – Au 5s – Cd 4s – Te 4p – Ce 4d – Rb 3d – Ni 3s – Pr 4d – At 5p – Bi 5p – Al 2s

Auger Energies #

Note – these are listed in KINETIC ENERGY

 

Be KLL ≈ 100 eV

Common Binding Energies – Be 1s #

 

Species #

Be Metal

BeO

BeCO3

Be2N

Be3N2

B.E. / eV #

110.5

113.5

114.7

111.3

113.8

Charge Ref #

C 1s (285 eV)

C 1s (285 eV)

C 1s (285 eV)

C 1s (285 eV)

C 1s (285 eV)

Reference #

Theory and Background #

Beryllium has a very low sensitivity in XPS, owing to very unfavourable photoionisation cross-sections (in fact, only Lithium has a lower cross-section).

As such it will be challenging to detect in low contents.

Experimental Advice #

Given the relatively low separation between multiple states, and the low intensity of the peaks owing to the unfavourable cross-sections, it can be advantageous to record the Be KLL auger also, since the Wagner plot of Be compounds may offer additional assistance in speciation.

See the work of Mallinson, Castle and Watts for more information.

 

Data Analysis Guidance #

Beryllium metal exhibits little asymmetry, and can be fit with a standard Voigt lineshape

 

Reference Datasets #

 

Coming soon

References #

  1. Mallinson, Christopher F., and James E. Castle. “Beryllium and beryllium oxide by XPS.” Surface Science Spectra 20.1 (2013): 86-96. Read it online here.
  2. Mallinson, Christopher F., James E. Castle, and John F. Watts. “The chemical state plot for beryllium compounds.” Surface and Interface Analysis 47.10 (2015): 994-995. Read it online here.