Tip‐Enhanced Resonance Couplings Revealed by High Vacuum Tip‐Enhanced Raman Spectroscopy
Source abstract
Abstract
Tip‐enhanced resonance couplings (TERCs) are experimentally revealed by high vacuum tip‐enhanced Raman spectroscopy (HV‐TERS) and theoretically interpreted. The Fermi resonance and Darling–Dennison resonance are successfully observed in HV‐TERS, which are the first overtone (or combinational mode)‐fundamental interaction (2:1 resonance coupling) and the first overtone‐first overtone resonant interaction (1:1 resonance coupling), respectively. The electric field gradient plays an important role on TERCs in HV‐TERS at the level of the second‐order perturbation theory. The molecular tautomeric effects are also observed from thiourea adsorbed on Ag film in HV‐TERS. The reported HERCs can provide a deeper understanding of the importance of molecular anharmonicity in high‐order perturbation for TERS. HV‐TER spectra provide ‘additional’ nonlinear Raman peaks, compared with the harmonic zero‐order perturbation in HV‐TERS, and thus enable ultrasensitive chemical analysis at the nanoscale with more vibrational information.
Source: crossref · Quality: baseline
Research context
OpenAlex topics: Spectroscopy and Quantum Chemical Studies · Protein Interaction Studies and Fluorescence Analysis · Photochemistry and Electron Transfer Studies
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Beijing National Laboratory for Condensed Matter Physics Institute of Physics Chinese Academy of Sciences PO Box 603–146 Beijing 100190 PR China
School of Physics & Technology Wuhan University Wuhan 430072 PR China
References (31)
Show source-provided references
1. 10.1016/S0009-2614(99)01451-710.1016/S0009-2614(99)01451-7 ↗
2. 10.1063/1.12654610.1063/1.126546 ↗
3. 10.1016/S0030-4018(00)00894-410.1016/S0030-4018(00)00894-4 ↗
4. 10.1146/annurev-physchem-032511-14380710.1146/annurev-physchem-032511-143807 ↗
5. 10.1039/C1NR11143D10.1039/C1NR11143D ↗
6. 10.1039/b705967c10.1039/b705967c ↗
7. 10.1002/anie.20080160510.1002/anie.200801605 ↗
8. 10.1039/c1cc13291a10.1039/c1cc13291a ↗
9. 10.1021/ja065820b10.1021/ja065820b ↗
10. 10.1103/PhysRevLett.100.23610110.1103/PhysRevLett.100.236101 ↗
11. 10.1021/jp209982h10.1021/jp209982h ↗
12. 10.1063/1.279422710.1063/1.2794227 ↗
13. 10.1038/srep0064710.1038/srep00647 ↗
14. 10.1021/nl203992510.1021/nl2039925 ↗
15. 10.1002/9780470143582.ch210.1002/9780470143582.ch2 ↗
16. 10.1007/BF0134171210.1007/BF01341712 ↗
17. 10.1103/PhysRevE.87.02040110.1103/PhysRevE.87.020401 ↗
18. 10.1103/PhysRev.57.12810.1103/PhysRev.57.128 ↗
19. 10.1039/c2ra21627b10.1039/c2ra21627b ↗
20. 10.1146/annurev.pc.46.100195.00214310.1146/annurev.pc.46.100195.002143 ↗
21. 10.1126/science.108917110.1126/science.1089171 ↗
22. Our home‐made TERS works well in high vacuum. It is difficult to perform the investigation on TERCs from TER spectra at ambient conditions because of two reasons: Firstly the high vacuum is difficult to recover well once it has been adjusted to ambient conditions. Secondly we are afraid that our home‐made HV‐TERS would be damaged in these processes.
23. 10.1063/1.168844210.1063/1.1688442 ↗
24. Kunz K. S. · 1993
25. FDTD Solutions · 2011
26. 10.1016/B978-0-08-054721-3.50037-X10.1016/B978-0-08-054721-3.50037-X ↗
27. 10.1007/978-3-642-86105-510.1007/978-3-642-86105-5 ↗
28. 10.1103/PhysRevB.54.1653310.1103/PhysRevB.54.16533 ↗
29. 10.1063/1.44879910.1063/1.448799 ↗
30. 10.1002/jrs.209310.1002/jrs.2093 ↗
31. Frisch M. J. · 2009