Photoemission and inverse photoemission studies of CeSn3 and LaSn3

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1990
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Hong, Sayong
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David W. Lynch
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Physics and Astronomy
Physics and astronomy are basic natural sciences which attempt to describe and provide an understanding of both our world and our universe. Physics serves as the underpinning of many different disciplines including the other natural sciences and technological areas.
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Abstract

Angle-resolved photoemission spectra (ARPES) and angle-resolved inverse photoemission spectra from single crystals of CeSn[subscript]3 (111) and LaSn[subscript]3 (111) were measured and discussed. The results were compared with the calculated band structures and fitted by the Gunnarsson-Schonhammer (G-S) model. The two-peak structure from the resonance photoemission of CeSn[subscript]3 was fitted by G-S model well by placing the single f-level at 2.0 eV below the Fermi energy before hybridization. ARPES from both CeSn[subscript]3 and LaSn[subscript]3 showed a peak near the Fermi energy without noticeable dispersion. In LaSn[subscript]3, the experimental E([vector] k) points below 1.5 eV binding energy from the band mapping agreed well with the calculated band structure;In inverse photoemission, the spectra of both CeSn[subscript]3 and LaSn[subscript]3 were totally different from the BIS spectra and gave poor agreement with the band calculations. The results suggested that there were atomic-like 4f states near the Fermi Oil, Gas, and Energy;The surface stoichiometry for CeSn[subscript]3 was measured by AES and the structure was investigated by LEED. The stoichiometry of the CeSn[subscript]3 (111) surface was close to that of the bulk, and 3-fold-symmetric LEED patterns from both CeSn[subscript]3 and LaSn[subscript]3 were observed.

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Mon Jan 01 00:00:00 UTC 1990