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X-ray versus Auger emission following Xe 1s photoionization
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Molecular and Condensed Matter Physics. UPMC Univ Paris 06, Sorbonne Univ, CNRS, UMR 7614,Lab Chim Phys Mat & Rayonnement, F-75005 Paris, France.;RIKEN SPring 8 Ctr, 1-1-1 Kouto, Sayo, Hyogo 6795148, Japan..
Univ Oulu, Nano & Mol Syst Res Unit, Box 3000, FI-90014 Oulu, Finland..
UPMC Univ Paris 06, Sorbonne Univ, CNRS, UMR 7614,Lab Chim Phys Mat & Rayonnement, F-75005 Paris, France.;RIKEN SPring 8 Ctr, 1-1-1 Kouto, Sayo, Hyogo 6795148, Japan..
RIKEN SPring 8 Ctr, 1-1-1 Kouto, Sayo, Hyogo 6795148, Japan.;Univ Hyogo, Grad Sch Mat Sci, Kamigori 6781297, Japan..
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2017 (English)In: Physical Review A. Atomic, Molecular, and Optical Physics, ISSN 1050-2947, E-ISSN 1094-1622, Vol. 95, no 6, article id 061402Article in journal (Refereed) Published
Abstract [en]

Xe 1s photoelectron spectra were measured at SPring-8, Japan. The core-hole lifetime broadening was found to be 9.6 eV, yielding a lifetime of similar to 68 as. The amount of radiative versus nonradiative decay was assessed by recording Auger LMM spectra below and above the K edge. Below the K edge, L vacancies are produced only by direct photoionization, while above the K edge some of these vacancies are mainly produced by KL emission following 1s photoionization. Due to the dipole selection rule for x-ray emission, the dominant role of the KL relaxation process is rather directly observed.

Place, publisher, year, edition, pages
2017. Vol. 95, no 6, article id 061402
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Atom and Molecular Physics and Optics
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URN: urn:nbn:se:uu:diva-327372DOI: 10.1103/PhysRevA.95.061402ISI: 000403219600001OAI: oai:DiVA.org:uu-327372DiVA, id: diva2:1130598
Available from: 2017-08-10 Created: 2017-08-10 Last updated: 2017-08-10Bibliographically approved

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Piancastelli, Maria Novella

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