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| Home > Publications database > Atomic-layer-resolved composition and electronic structure of the cuprate B i 2 S r 2 CaC u 2 O 8 + δ from soft x-ray standing-wave photoemission > print |
| Home > Publications database > Atomic-layer-resolved composition and electronic structure of the cuprate B i 2 S r 2 CaC u 2 O 8 + δ from soft x-ray standing-wave photoemission > print |
| 001 | 859706 | ||
| 005 | 20230426083204.0 | ||
| 024 | 7 | _ | |a 10.1103/PhysRevB.98.155133 |2 doi |
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| 100 | 1 | _ | |a Kuo, Cheng-Tai |0 P:(DE-HGF)0 |b 0 |e Corresponding author |
| 245 | _ | _ | |a Atomic-layer-resolved composition and electronic structure of the cuprate B i 2 S r 2 CaC u 2 O 8 + δ from soft x-ray standing-wave photoemission |
| 260 | _ | _ | |a Woodbury, NY |c 2018 |b Inst. |
| 336 | 7 | _ | |a article |2 DRIVER |
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| 520 | _ | _ | |a A major remaining challenge in the superconducting cuprates is the unambiguous differentiation of the composition and electronic structure of the CuO2 layers and those of the intermediate layers. The large c axis for these materials permits employing soft x-ray (930.3 eV) standing wave (SW) excitation in photoemission that yields atomic layer-by-layer depth resolution of these properties. Applying SW photoemission to Bi2Sr2CaCu2O8+δ yields the depth distribution of atomic composition and the layer-resolved densities of states. We detect significant Ca presence in the SrO layers and oxygen bonding to three different cations. The layer-resolved valence electronic structure is found to be strongly influenced by the atomic supermodulation structure, as determined by comparison to density functional theory calculations, by Ca-Sr intermixing, and by correlation effects associated with the Cu 3d−3d Coulomb interaction, further clarifying the complex interactions in this prototypical cuprate. Measurements of this type for other quasi-two-dimensional materials with large c represent a promising future direction. |
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| 773 | 1 | 8 | |a 10.1103/physrevb.98.155133 |b American Physical Society (APS) |d 2018-10-19 |n 15 |p 155133 |3 journal-article |2 Crossref |t Physical Review B |v 98 |y 2018 |x 2469-9950 |
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