2009
DOI: 10.1016/j.elspec.2008.11.004
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A systematic study of photoionization of free lanthanide atoms in the 4d giant resonance region

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Cited by 6 publications
(5 citation statements)
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“…Photoabsorption [16][17][18][19], electron scattering [20,21], and inelastic x-ray scattering [22] by lanthanides near the 3d and 4d electron edges are important tools for understanding magnetic materials. They reveal atomic-like 4f features that show effects of orbital collapse similar to those we study here.…”
Section: Introductionmentioning
confidence: 99%
“…Photoabsorption [16][17][18][19], electron scattering [20,21], and inelastic x-ray scattering [22] by lanthanides near the 3d and 4d electron edges are important tools for understanding magnetic materials. They reveal atomic-like 4f features that show effects of orbital collapse similar to those we study here.…”
Section: Introductionmentioning
confidence: 99%
“…As described by Filevich et al [13], EUV emission from laser-produced plasmas creates a cold plasma on the target surface dominated by low ion stages. As the photoabsorption profile of neutral to 3 times ionized Gd consists of giant resonances in the 7−9 nm range with cross sections up to tens of Mb [14][15][16], radiation trapping by low ion stages may considerably reduce the observed intensity in this region. …”
mentioning
confidence: 99%
“…However, the 5d and 6s emissions can be clearly distinguished from the 4f emission from free atoms of rare earth metals by photoelectron spectroscopy. [10,11] The divalent and trivalent features of the spectra presented here are of the Sm over-layers with coverage higher than 1.0 Å. These features are different in comparison to those of the Sm over-layers on singlecrystal substrate systems of Sm/Ta (110) and Sm/Mo.…”
Section: Resultsmentioning
confidence: 84%
“…[17,18] At a low coverage of 0.3-0.6 Å, the global feature of the 4f emission spectra is comparable with the spectrum of the free Sm atom with an initial divalent state of 4f 6 6s 2 . [10] The 4f 5 and 4f 4 multiplet features coexist in the spectra of the Sm over-layers with coverage in the range of 1.0-5.0 Å. This is because the component of the trivalent Sm becomes larger with increasing coverage of the Sm over-layer.…”
Section: Resultsmentioning
confidence: 93%