journal article·2017-03-28Open access

Two-Orbital Kondo Screening in a Self-Assembled Metal–Organic Complex

Giulia E. Pacchioni, Marina Pivetta, Luca Gragnaniello, Fabio Donati, Gabriel Autès, Oleg V. Yazyev, Stefano Rusponi, Harald Brune

ACS Nano· Volume 11· Issue 3

Abstract

Iron atoms adsorbed on a Cu(111) surface and buried under polyphenyl dicarbonitrile molecules exhibit strongly spatial anisotropic Kondo features with directionally dependent Kondo temperatures and line shapes, as evidenced by scanning tunneling spectroscopy. First-principles calculations find nearly full polarization for the half-filled Fe 3d xz and 3d yz orbitals, which therefore can give rise to Kondo screening with the experimentally observed directional dependence and distinct Kondo temperatures. X-ray absorption spectroscopy and X-ray magnetic circular dichroism measurements confirm that the spin in both channels is effectively Kondo-screened. At ideal Fe coverage, these two-orbital Kondo impurities are arranged in a self-assembled honeycomb superlattice.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Quantum and electron transport phenomena · Advanced Chemical Physics Studies · Magnetic properties of thin films

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

Institute of Physics, Ecole Polytechnique Fédérale de Lausanne (EPFL), CH-1015 Lausanne, Switzerland

Funding

Schweizerischer Nationalfonds zur F?rderung der Wissenschaftlichen Forschung

References (46)

Show source-provided references
1. 10.1143/PTP.32.3710.1143/PTP.32.37 ↗
2. 10.1126/science.280.5363.56710.1126/science.280.5363.567 ↗
3. 10.1038/3500050810.1038/35000508 ↗
4. 10.1088/0953-8984/21/5/05300110.1088/0953-8984/21/5/053001 ↗
5. 10.1038/3437310.1038/34373 ↗
6. 10.1126/science.281.5376.54010.1126/science.281.5376.540 ↗
7. 10.1038/nmat213310.1038/nmat2133 ↗
8. 10.1021/nn100793s10.1021/nn100793s ↗
9. 10.1021/nl301301e10.1021/nl301301e ↗
10. 10.1021/ja303510g10.1021/ja303510g ↗
11. 10.1021/nn403959510.1021/nn4039595 ↗
12. 10.1038/srep0121010.1038/srep01210 ↗
13. 10.1103/PhysRevLett.113.10610210.1103/PhysRevLett.113.106102 ↗
14. 10.1126/science.111344910.1126/science.1113449 ↗
15. 10.1103/PhysRevLett.101.21720310.1103/PhysRevLett.101.217203 ↗
16. 10.1021/acsnano.5b0612010.1021/acsnano.5b06120 ↗
17. 10.1021/nl102456310.1021/nl1024563 ↗
18. 10.1038/ncomms121010.1038/ncomms1210 ↗
19. 10.1103/PhysRevLett.116.02720110.1103/PhysRevLett.116.027201 ↗
20. 10.1038/ncomms149710.1038/ncomms1497 ↗
21. 10.1126/science.120220410.1126/science.1202204 ↗
22. 10.1103/PhysRevLett.109.14720210.1103/PhysRevLett.109.147202 ↗
23. 10.1103/PhysRevB.91.04544010.1103/PhysRevB.91.045440 ↗
24. 10.1021/nl072466m10.1021/nl072466m ↗
25. 10.1021/acs.jpcc.5b0864410.1021/acs.jpcc.5b08644 ↗
26. 10.1103/PhysRevLett.110.08610210.1103/PhysRevLett.110.086102 ↗
27. 10.1021/nl802677c10.1021/nl802677c ↗
28. 10.1002/adfm.20100194010.1002/adfm.201001940 ↗
29. 10.1103/PhysRevLett.106.20680310.1103/PhysRevLett.106.206803 ↗
30. 10.1103/PhysRev.124.186610.1103/PhysRev.124.1866 ↗
31. 10.1103/PhysRevLett.88.07720510.1103/PhysRevLett.88.077205 ↗
32. 10.1038/nphys107210.1038/nphys1072 ↗
33. 10.1103/PhysRevLett.105.10660110.1103/PhysRevLett.105.106601 ↗
34. 10.1103/PhysRevLett.88.09680410.1103/PhysRevLett.88.096804 ↗
35. 10.1021/nl404054v10.1021/nl404054v ↗
36. 10.1103/PhysRevB.44.94310.1103/PhysRevB.44.943 ↗
37. 10.1088/0953-8984/21/39/39550210.1088/0953-8984/21/39/395502 ↗
38. 10.1002/jcc.2049510.1002/jcc.20495 ↗
39. 10.1002/jcc.2111210.1002/jcc.21112 ↗
40. 10.1063/1.174763210.1063/1.1747632 ↗
41. 10.1021/nl501150k10.1021/nl501150k ↗
42. 10.1103/PhysRevLett.85.255710.1103/PhysRevLett.85.2557 ↗
43. 10.1103/PhysRevB.92.04511910.1103/PhysRevB.92.045119 ↗
44. 10.1107/S090904951202784710.1107/S0909049512027847 ↗
45. 10.1103/PhysRevB.91.23542610.1103/PhysRevB.91.235426 ↗
46. 10.1016/0304-3991(92)90495-610.1016/0304-3991(92)90495-6 ↗