This work was partly carried out while one of us (JRL) was a visiting scientist at the Academy of Fine Arts, Vienna.
Research Article
Surface-enhanced Raman spectroscopy of indanthrone and flavanthrone
Article first published online: 12 JUN 2009
DOI: 10.1002/jrs.2298
Copyright © 2009 John Wiley & Sons, Ltd.
Additional Information
How to Cite
Chang, J., Cañamares, M. V., Aydin, M., Vetter, W., Schreiner, M., Xu, W. and Lombardi, J. R. (2009), Surface-enhanced Raman spectroscopy of indanthrone and flavanthrone. J. Raman Spectrosc., 40: 1557–1563. doi: 10.1002/jrs.2298
Publication History
- Issue published online: 11 NOV 2009
- Article first published online: 12 JUN 2009
- Manuscript Accepted: 9 MAR 2009
- Manuscript Received: 28 JAN 2009
Funded by
- National Science Foundation. Grant Numbers: CHE-0091362, CHE-0345987, ECS0217646
- National Natural Science Foundation of China. Grant Numbers: NSFC 20773045, 20627002
Keywords:
- Flavanthrone;
- Indanthrone;
- SERS;
- DFT
Abstract
The normal Raman and surface-enhanced Raman scattering (SERS) spectra of flavanthrone and indanthrone were obtained at several excitation wavelengths. The spectral assignments were aided by density functional calculations. Since both molecules have very high symmetry (C2h) including a center of inversion, we expect that the modes of u symmetry will be forbidden in the normal Raman spectrum. However, proximity to the surface causes special SERS enhancement of several of the bu modes, along with somewhat weaker enhancement of the au and bg modes. Copyright © 2009 John Wiley & Sons, Ltd.

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