1996
DOI: 10.1103/physrevb.54.r15618
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Magnetic dichroism in photoemission as a spin-resolving probe for electronic correlations

Abstract: Magnetic dichroism with unpolarized x rays in angle-resolved photoemission has been systematically investigated for the 2p core levels of Fe, Co, and Ni. In contrast to Fe 2p, we find the dichroism in the Ni 2p spectra to be mainly governed by electronic correlations. The fine structure observed in the Co 2p spectrum indicates a distinct influence of many-body interactions also in this material. ͓S0163-1829͑96͒50446-7͔Electronic interactions govern many phenomena in solidstate physics. Ferromagnetism, for inst… Show more

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Cited by 34 publications
(28 citation statements)
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References 27 publications
(34 reference statements)
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“…An alternative interpretation of the high binding energy emission in the Co 2p 3/2 line shape might be in terms of a correlation-induced shake-up satellite, which is caused by the screening of a two-d-hole c À1 3d 8 4s 2 final state (c À1 is the core hole) by the conduction electrons [20]. This satellite structure is located at about 4.5 eV from the main emission line (c À1 3d 9 4s 1 ) and its spectral weight was shown to be crucially dependent on the Co dimensions: whereas the satellite intensity is hardly distinguished in Co 2p spectra of bulk samples, it may become significantly enhanced in systems with reduced dimensions, as recently demonstrated for Co nanolayers on Cu(1 0 0) and OCu(1 0 0) surfaces [21][22][23]. Theoretical results have predicted that the spectral weight of the shake-up satellite becomes significant in the case of strong d-d correlation and dehybridisation of the Co 3d bands [24,25].…”
Section: Resultsmentioning
confidence: 82%
“…An alternative interpretation of the high binding energy emission in the Co 2p 3/2 line shape might be in terms of a correlation-induced shake-up satellite, which is caused by the screening of a two-d-hole c À1 3d 8 4s 2 final state (c À1 is the core hole) by the conduction electrons [20]. This satellite structure is located at about 4.5 eV from the main emission line (c À1 3d 9 4s 1 ) and its spectral weight was shown to be crucially dependent on the Co dimensions: whereas the satellite intensity is hardly distinguished in Co 2p spectra of bulk samples, it may become significantly enhanced in systems with reduced dimensions, as recently demonstrated for Co nanolayers on Cu(1 0 0) and OCu(1 0 0) surfaces [21][22][23]. Theoretical results have predicted that the spectral weight of the shake-up satellite becomes significant in the case of strong d-d correlation and dehybridisation of the Co 3d bands [24,25].…”
Section: Resultsmentioning
confidence: 82%
“…The most prominent one is the sensitivity of MLDAD on the transverse component of the magnetization, well known from numerous photoemission experiments. [11][12][13][14][15][16][17][18][19][20][21][22][23][24][25][26][27][28] This is even true for excitation by circularly polarized light, 7 where the intensity asymmetry for different kinetic energies depends on both the longitudinal and the transverse components. This is due to the fact that for circular polarization a mixture of two effects contributes to this asymmetry, 28 -32 one being the linear dichroism displayed in Fig.…”
Section: Discussionmentioning
confidence: 98%
“…5 If energy filtering of photoemitted electrons is possible, magnetic dichroisms which occur in photoelectron spectroscopy may be employed as magnetic contrast mechanisms. Such dichroisms occur for various experimental geometries that involve circularly, 6-10 linearly, [10][11][12][13][14][15][16][17][18][19] or even unpolarized light, [20][21][22][23][24][25][26][27] and they can be observed in valence band 6,7,[17][18][19][20]28 or core level photoemission spectra. 8 -16,21-27 For highly symmetric geometries, circular dichroism in photoemission can be described in terms of relativistic selection rules for transitions between exchange and spin-orbit split states.…”
Section: Introductionmentioning
confidence: 99%
“…In addition, satellite features at 3.7, 27.2, and 42.7 eV above the 2p 3/2 peak are indicated by downward pointing arrows. These satellites have been discussed previously, 15,16 with the 3.7 eV feature being ascribed to a two-hole final state in an analogous manner to the case for Ni XPS satellites. 14 The MCDPE spectrum, which is the difference between the two displayed XPS spectra, is also shown in Fig.…”
mentioning
confidence: 94%
“…This line shape is similar to that reported by Dürr et al 17 for Fe thin films grown on Cu͑001͒ which could not be reproduced by one-electron calculations. From the similarity between the Fe MCDPE 15,17 and the Co MCDPE presented in this work it can be expected that a one-electron approach will also fail to reproduce the Co MCDPE. For the latter this is in part due to the electron correlation features in the MCDPE which are not considered in a one-electron approach.…”
mentioning
confidence: 99%