Atomic multiplet and charge transfer screening effects in 1s and 2p core-level x-ray photoelectron spectra of early 3d transition-metal oxides
Source abstract
Abstract
We present a comparative analysis of $1s$ and $2p$ core-level hard x-ray photoelectron spectroscopy (HAXPES) spectra of metallic ${\mathrm{VO}}2$ and ${\mathrm{CrO}}2$. Even though the V $1s$ and $2p$ spectra in ${\mathrm{VO}}2$ show similar line shapes except for the absence/presence of a spin-orbit splitting in the core levels, the Cr $1s$ and $2p$ spectra exhibit distinct main-line shapes. The experimental HAXPES spectra are analyzed by the Anderson impurity model based on the density functional theory $+$ dynamical mean-field theory and a conventional ${\mathrm{MO}}6$ cluster model. We examine the interplay between the formation of the intra-atomic multiplet between a core hole and valence electrons and the charge-transfer effect on the chemical bonding followed by the $1s$ and $2p$ core electron excitations. We demonstrate the advantage of $1s$ HAXPES to the routinely employed $2p$ one for distinguishing contributions of a metal-ligand and metallic screening from a state near the Fermi level in metallic early $3d$ transition-metal oxides.
Source: openalex_inverted_index · Quality: baseline
Research context
OpenAlex topics: Transition Metal Oxide Nanomaterials · Catalysis and Oxidation Reactions · Ga2O3 and related materials
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Osaka Metropolitan University 1-1 Gakuen-cho
University College London
Utrecht University
Funding
Japan Society for the Promotion of Science
References (62)
Show source-provided references
1. 10.1103/RevModPhys.70.103910.1103/RevModPhys.70.1039 ↗
2. D. I. Khomskii · 201410.1017/CBO9781139096782 ↗
3. 10.1103/PhysRevLett.107.25640110.1103/PhysRevLett.107.256401 ↗
4. 10.1103/PhysRevLett.115.13640110.1103/PhysRevLett.115.136401 ↗
5. 10.1146/annurev-conmatphys-020911-12504510.1146/annurev-conmatphys-020911-125045 ↗
6. F. de Groot · 2008
7. 10.1103/PhysRevB.74.08511810.1103/PhysRevB.74.085118 ↗
8. 10.1103/PhysRevLett.70.245910.1103/PhysRevLett.70.2459 ↗
9. 10.1103/PhysRevB.100.07514610.1103/PhysRevB.100.075146 ↗
10. 10.1016/j.elspec.2013.01.00510.1016/j.elspec.2013.01.005 ↗
11. M. Taguchi · 2016
12. 10.1016/j.elspec.2015.07.00510.1016/j.elspec.2015.07.005 ↗
13. 10.1088/1361-648X/abeacd10.1088/1361-648X/abeacd ↗
14. 10.1016/j.nima.2008.12.18810.1016/j.nima.2008.12.188 ↗
15. 10.1103/PhysRevB.97.23514810.1103/PhysRevB.97.235148 ↗
16. 10.1103/PhysRevB.101.24511910.1103/PhysRevB.101.245119 ↗
17. 10.1103/PhysRevB.91.20141210.1103/PhysRevB.91.201412 ↗
18. 10.1103/PhysRevB.106.20513810.1103/PhysRevB.106.205138 ↗
19. 10.1103/PhysRevB.96.04511110.1103/PhysRevB.96.045111 ↗
20. 10.1103/PhysRevLett.93.23640110.1103/PhysRevLett.93.236401 ↗
21. 10.1103/PhysRevLett.104.10640110.1103/PhysRevLett.104.106401 ↗
22. 10.1103/PhysRevB.71.15510210.1103/PhysRevB.71.155102 ↗
23. 10.1103/PhysRevB.78.07511510.1103/PhysRevB.78.075115 ↗
24. 10.1088/1367-2630/11/10/10301510.1088/1367-2630/11/10/103015 ↗
25. 10.1103/PhysRevLett.124.19640210.1103/PhysRevLett.124.196402 ↗
26. 10.1103/PhysRevLett.95.17700210.1103/PhysRevLett.95.177002 ↗
27. 10.1209/0295-5075/108/5700410.1209/0295-5075/108/57004 ↗
28. 10.1103/PhysRevB.75.11511210.1103/PhysRevB.75.115112 ↗
29. 10.1103/PhysRevB.87.23513810.1103/PhysRevB.87.235138 ↗
30. 10.1038/s41467-023-41816-310.1038/s41467-023-41816-3 ↗
31. 10.1038/nphys273310.1038/nphys2733 ↗
32. 10.1103/PhysRevB.108.04511210.1103/PhysRevB.108.045112 ↗
33. 10.1103/PhysRevLett.121.25720110.1103/PhysRevLett.121.257201 ↗
34. 10.1088/1361-648X/ac7f1810.1088/1361-648X/ac7f18 ↗
35. 10.1103/RevModPhys.68.1310.1103/RevModPhys.68.13 ↗
36. 10.1103/RevModPhys.78.86510.1103/RevModPhys.78.865 ↗
37. 10.1140/epjst/e2010-01209-010.1140/epjst/e2010-01209-0 ↗
38. 10.1103/PhysRevB.88.08512310.1103/PhysRevB.88.085123 ↗
39. 10.1103/PhysRevB.10.49010.1103/PhysRevB.10.490 ↗
40. P. Blaha · 2018
41. 10.1016/j.cpc.2010.08.00510.1016/j.cpc.2010.08.005 ↗
42. 10.1016/j.cpc.2014.05.00310.1016/j.cpc.2014.05.003 ↗
43. 10.1103/PhysRevLett.90.23720310.1103/PhysRevLett.90.237203 ↗
44. 10.1103/PhysRevLett.117.05640210.1103/PhysRevLett.117.056402 ↗
45. 10.1103/PhysRevLett.97.07640510.1103/PhysRevLett.97.076405 ↗
46. 10.1103/PhysRevB.84.07514510.1103/PhysRevB.84.075145 ↗
47. 10.1103/PhysRevB.85.20510610.1103/PhysRevB.85.205106 ↗
48. 10.7566/JPSJ.84.07370610.7566/JPSJ.84.073706 ↗
49. 10.1016/j.elspec.2010.05.02110.1016/j.elspec.2010.05.021 ↗
50. 10.1016/0370-1573(95)00074-710.1016/0370-1573(95)00074-7 ↗
51. 10.1103/PhysRevLett.3.3410.1103/PhysRevLett.3.34 ↗
52. 10.1063/1.200047710.1063/1.2000477 ↗
53. 10.1103/PhysRevB.102.08515510.1103/PhysRevB.102.085155 ↗
54. 10.1103/PhysRevB.42.545910.1103/PhysRevB.42.5459 ↗
55. 10.1143/JPSJ.74.205210.1143/JPSJ.74.2052 ↗
56. 10.1103/PhysRevB.5.178510.1103/PhysRevB.5.1785 ↗
57. 10.1143/JPSJ.61.204010.1143/JPSJ.61.2040 ↗
58. 10.1103/PhysRevB.101.11513010.1103/PhysRevB.101.115130 ↗
59. 10.1016/S0368-2048(96)03063-010.1016/S0368-2048(96)03063-0 ↗
60. 10.1103/PhysRevLett.94.02640410.1103/PhysRevLett.94.026404 ↗
61. 10.1143/JPSJ.62.259510.1143/JPSJ.62.2595 ↗
62. 10.1103/PhysRevB.71.05240710.1103/PhysRevB.71.052407 ↗