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The types of state-to-state transitions available to electrons during an Auger event are dependent on several factors, ranging from initial excitation energy to relative interaction rates, yet are often dominated by a few characteristic transitions.
Because of the interaction between an electron's spin and orbital angular momentum ( spin-orbit coupling ) and the concomitant energy level splitting for various shells in an atom, there are a variety of transition pathways for filling a core hole.
Energy levels are labeled using a number of different schemes such as the j-j coupling method for heavy elements ( Z ≥ 75 ), the Russell-Saunders L-S method for lighter elements ( Z < 20 ), and a combination of both for intermediate elements.
The j-j coupling method, which is historically linked to X-ray notation, is almost always used to denote Auger transitions.
Thus for a transition, K represents the core level hole, the relaxing electron's initial state, and the emitted electron's initial energy state.
For single energy levels, i. e. K, transitions can occur from the L levels, giving rise to strong KLL type peaks in an Auger spectrum.
For multi-level shells, transitions are available from higher energy orbitals ( different n, ℓ quantum numbers ) or energy levels within the same shell ( same n, different ℓ number ).
The result are transitions of the type LMM and KLL along with faster Coster – Kronig transitions such as LLM.
while Coster – Kronig transitions are faster, they are also less energetic and thus harder to locate on an Auger spectrum.
Fortunately, the strongest electron-electron interactions are between levels which are close together, giving rise to characteristic peaks in an Auger spectrum.
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