2015
DOI: 10.1103/physrevlett.114.093001
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Direct Observation of Double-Core-Hole Shake-Up States in Photoemission

Abstract: Direct measurements of Ar^{+} 1s^{-1}2p^{-1}nl double-core-hole shake-up states are reported using conventional single-channel photoemission, offering a new and relatively easy means to study such species. The high-quality results yield accurate energies and lifetimes of the double-core-hole states. Their photoemission spectrum also can be likened to 1s absorption of an exotic argon ion with a 2p core vacancy, providing new information about the spectroscopy of both this unusual ionic state as well as the neut… Show more

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Cited by 41 publications
(77 citation statements)
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References 29 publications
(50 reference statements)
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“…The model threshold energies for 1s + 2s and 1s + 1s double detachment are slightly higher than the calculated threshold energies from Table I for these processes. We attribute this to the fact that the sudden change of the atomic potential following double detachment gives rise to a sizeable shake-up of L-shell electrons as has explicitly been shown, e.g., by Auger electron and photoelectron spectroscopy of double core-hole levels of rare-gas atoms [27][28][29]. The present structure calculations suggest that shake-up processes can shift the double-detachment thresholds of C − to higher energies by up to 20 eV.…”
supporting
confidence: 66%
“…The model threshold energies for 1s + 2s and 1s + 1s double detachment are slightly higher than the calculated threshold energies from Table I for these processes. We attribute this to the fact that the sudden change of the atomic potential following double detachment gives rise to a sizeable shake-up of L-shell electrons as has explicitly been shown, e.g., by Auger electron and photoelectron spectroscopy of double core-hole levels of rare-gas atoms [27][28][29]. The present structure calculations suggest that shake-up processes can shift the double-detachment thresholds of C − to higher energies by up to 20 eV.…”
supporting
confidence: 66%
“…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%
“…Around the same time, Lablanquie and coworkers 6 presented similar studies on N 2 , CO, CO 2 and O 2 . Building on the works of Eland et al 3 and Lablanquie et al, 6 Püttner et al 8 and Goldsztejn et al 9 showed more recently that DCH states of the pre-edge type can also be observed using a high resolution single-channel electron spectroscopy technique for detecting the one core electron which gets ejected into the continuum at a very well defined kinetic energy. With this technique they were able to detect DCH states with binding energies up to 3.5 keV.…”
Section: Introductionmentioning
confidence: 99%