2017
DOI: 10.1103/physrevlett.119.263003
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Ultrafast Charge Transfer Processes Accompanying KLL Auger Decay in Aqueous KCl Solution

Abstract: X-ray photoelectron spectroscopy (XPS) and KLL Auger spectra of aqueous KCl solution were measured for the K + and Cledges. While the XPS spectra of potassium and chloride have similar structures, both exhibiting only weak satellite structures near the main line, the Auger spectra of these isoelectronic ions differ dramatically. A very strong satellite peak was found in the K + KLL Auger spectrum at the low kinetic energy side of the 1 D state. Using equivalent core models and ab initio calculations this spect… Show more

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Cited by 11 publications
(10 citation statements)
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References 48 publications
(60 reference statements)
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“…the resolving power E/ΔE higher than 5000 (where E is the kinetic energy of electron and ΔE the instrumental resolution), are quite scarce. Up to now, the GALAXIES beamline at the SOLEIL synchrotron [2,3] has been the only facility for high-resolution HAXPES experiments on atomic and molecular science and has been achieving significant results on double-core-hole spectroscopy [4][5][6][7], recoil effects [8][9][10], ultrafast phenomena [11][12][13], post-collision interaction (PCI) [14,15], resonant Auger processes [16][17][18][19][20], and very recent studies on aqueous solution [21,22]. The experiments at the GALAXIES beamline, however, are limited to the excitation energy ranging between 2.3 and 12 keV, while experiments with much higher photon energy are quite scarce.…”
Section: Introductionmentioning
confidence: 99%
“…the resolving power E/ΔE higher than 5000 (where E is the kinetic energy of electron and ΔE the instrumental resolution), are quite scarce. Up to now, the GALAXIES beamline at the SOLEIL synchrotron [2,3] has been the only facility for high-resolution HAXPES experiments on atomic and molecular science and has been achieving significant results on double-core-hole spectroscopy [4][5][6][7], recoil effects [8][9][10], ultrafast phenomena [11][12][13], post-collision interaction (PCI) [14,15], resonant Auger processes [16][17][18][19][20], and very recent studies on aqueous solution [21,22]. The experiments at the GALAXIES beamline, however, are limited to the excitation energy ranging between 2.3 and 12 keV, while experiments with much higher photon energy are quite scarce.…”
Section: Introductionmentioning
confidence: 99%
“…[4][5][6][7][8] and references therein. Recently, electron transfer processes from solvent water molecules to the solvated cation in the hard-x-ray regime have been observed [9]. However, the simultaneous presence of electron and nuclear dynamics in x-ray-excited liquid water hinders the interpretation of the measurements.…”
Section: Introductionmentioning
confidence: 99%
“…Our analysis reveals that these dierences result to a large extent from dierent electronic structures of the two ions, thus conrming that the combination of XAS and AES techniques is a sensitive probe of the electronic structure of solutions. and 3(c)) and also shifted to higher kinetic energies as compared to the spectra reported in 16 . This is due to post-collision interaction 21,22 discussed in more detail in the SI.…”
mentioning
confidence: 54%
“…The position of the rst peak coincides with the 1 D main line resulting from normal Auger decay, whereas the second peak at 2383.5 eV corresponds to resonant Auger decay to the 2p −2 ( 1 D)4p states. The fast delocalization in this case is a result of the fact that the energy splitting between the Cl − (1s −1 4p) resonance and the ionization threshold is 0.2 eV, and thus, smaller than the lifetime broadening of 0.62 eV 16 .…”
mentioning
confidence: 84%
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