1995
DOI: 10.1103/physrevb.52.6057
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Mercury surface-plasmon dispersion: Experiment and theory

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Cited by 27 publications
(41 citation statements)
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“…Significant deviations from the dispersion of surface plasmons at jellium surfaces occur on the noble metal Ag [107,108,109,110], and the transition metals Hg [111] and Pd [297] (see Table IV). These deviations are mainly due to the presence in these metals of filled 4d and 5d bands, which in the case of Ag yields an anomalous positive and strongly crystal-face dependent dispersion.…”
Section: Occupied D-bands: Simple Modelsmentioning
confidence: 99%
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“…Significant deviations from the dispersion of surface plasmons at jellium surfaces occur on the noble metal Ag [107,108,109,110], and the transition metals Hg [111] and Pd [297] (see Table IV). These deviations are mainly due to the presence in these metals of filled 4d and 5d bands, which in the case of Ag yields an anomalous positive and strongly crystal-face dependent dispersion.…”
Section: Occupied D-bands: Simple Modelsmentioning
confidence: 99%
“…However, first-principles calculations of the surfaceplasmon energy and linewidth dispersion of real solids have been carried out only in the case of the simple-metal prototype surfaces Mg(0001) and Al (111) [121,122]. These calculations lead to an accurate description of the measured surface-plasmon energy dispersion that is superior to that obtained in the jellium model, and they show that the band structure is of paramount importance for a correct description of the surface-plasmon linewidth.…”
mentioning
confidence: 99%
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“…[1][2][3][4][5][6][7] The surface photoeffect is closely related to the excitation and the subsequent decay of the multiple surface plasmons, or multipole mode. [8][9][10][11][12][13] This mechanism of the enhancement of the surface photoemission is widely recognized and has been reported for clean surfaces and thin films of simple metals. 3,11,14,15 The mapping of the bulk band structure, using photoemission techniques, 7,[16][17][18] can be facilitated by enhanced cross section ͑and therefore more intense peaks in the photoemission spectra͒ through the Coster-Kronig resonant optical transitions, as allowed by the photoemission selection rules.…”
Section: Introductionmentioning
confidence: 99%