hereby m depends the atomic number Z of the medium and decreases with increasing photon energy hn [1]. However, the fine structure of this element-specific edge of the absorption coefficient is influenced by the energy of unoccupied electronic levels, as it is depicted in Fig. 1(a). Only a sufficient photon energy enables the photoexcitation of a core level electron beyond the vacuum level Evac. After 10×10-14 sec [2] the ionized atom may relax by occupation of the core hole with an electron from the valence band (VB), while the generated energy will normally not be used for the emission of a flourescence photon (probability 1 %), but will be absorbed for the vaccum emission of an Auger electron (probability 99%) from the valence band. In case of a non-sufficient energy for the emission of the primary electron, it may be excited into a conduction band (CB) level, so that a similar relaxation process becomes possible. This spectator process then results in the emission of only one Auger electron.
Alternatively the core hole may be reoccupied by the core level electron itself, so that the excitation energy is finally used for the emission of a valence electron. As the final state of this participator process is comparable to a direct photoemission process and as both mechanisms may happen concurently, the participator excitation is also called resonant photoemission.
The number of generated secondary electrons is thereby directly proportional to the x-ay absortion cross section [3]. On their way to the crystal surface these electrons undergo multiple scattering processes with other electrons (Fig. 1(b)), so that their number is multiplied while their averaged energy is reduced. Consequently, from the atomic layers near the surface up to 50 Å depth low-energy photolectrons are emitted. For the determination of the absorption coefficient m depending on the photon energy two techniques are possible. The integrated detection of all emitted electrons (total electron yield) as well as the selective detection of electrons of fixed energy (partial electron yield) as a function of hn will lead to equivalent structures in the spectra [4].
The typical XANES experiment measures the photoelectron intensity for photon energies beginning from the absorption edge til 50 eV beyond the edge energy [5]. Although photon energies below the ionization threshold allow electronic transitions into unoccupied elctronic bands or molecular orbitals, the spectral features are not directly related to the unoccupied density of states (UDOS) [6], which can be probed with inverse photoemission spectroscopy. In particular, p-conjugated molecular systems [7] exhibit a strong excitonic interaction between core electron and hole, so that the transitions show shifted energetic positions in the absorption spectra [8]. In case of an inhomogeneous intramolecular charge distribution the same electronic transition may even be found as slightly shifted double structures [9]. Nevertheless the well-structured molecular absorption spectra are a powerfull tool for the identifaction of chemical components and redox-induced changes.
References
hereby m depends the atomic number Z of the medium and decreases with increasing photon energy hn [1]. However, the fine structure of this element-specific edge of the absorption coefficient is influenced by the energy of unoccupied electronic levels, as it is depicted in Fig. 1(a). Only a sufficient photon energy enables the photoexcitation of a core level electron beyond the vacuum level Evac. After 10×10-14 sec [2] the ionized atom may relax by occupation of the core hole with an electron from the valence band (VB), while the generated energy will normally not be used for the emission of a flourescence photon (probability 1 %), but will be absorbed for the vaccum emission of an Auger electron (probability 99%) from the valence band. In case of a non-sufficient energy for the emission of the primary electron, it may be excited into a conduction band (CB) level, so that a similar relaxation process becomes possible. This spectator process then results in the emission of only one Auger electron.
Alternatively the core hole may be reoccupied by the core level electron itself, so that the excitation energy is finally used for the emission of a valence electron. As the final state of this participator process is comparable to a direct photoemission process and as both mechanisms may happen concurently, the participator excitation is also called resonant photoemission.
The number of generated secondary electrons is thereby directly proportional to the x-ay absortion cross section [3]. On their way to the crystal surface these electrons undergo multiple scattering processes with other electrons (Fig. 1(b)), so that their number is multiplied while their averaged energy is reduced. Consequently, from the atomic layers near the surface up to 50 Å depth low-energy photolectrons are emitted. For the determination of the absorption coefficient m depending on the photon energy two techniques are possible. The integrated detection of all emitted electrons (total electron yield) as well as the selective detection of electrons of fixed energy (partial electron yield) as a function of hn will lead to equivalent structures in the spectra [4].
The typical XANES experiment measures the photoelectron intensity for photon energies beginning from the absorption edge til 50 eV beyond the edge energy [5]. Although photon energies below the ionization threshold allow electronic transitions into unoccupied elctronic bands or molecular orbitals, the spectral features are not directly related to the unoccupied density of states (UDOS) [6], which can be probed with inverse photoemission spectroscopy. In particular, p-conjugated molecular systems [7] exhibit a strong excitonic interaction between core electron and hole, so that the transitions show shifted energetic positions in the absorption spectra [8]. In case of an inhomogeneous intramolecular charge distribution the same electronic transition may even be found as slightly shifted double structures [9]. Nevertheless the well-structured molecular absorption spectra are a powerfull tool for the identifaction of chemical components and redox-induced changes.
References
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