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dc.contributor.authorChang, Jingjing
dc.contributor.authorCanamares, Maria Vega
dc.contributor.authorAydin, Metin
dc.contributor.authorVetter, Wilfried
dc.contributor.authorSchreiner, Manfred
dc.contributor.authorXu, Weiqing
dc.contributor.authorLombardi, John R.
dc.date.accessioned2020-06-21T14:54:14Z
dc.date.available2020-06-21T14:54:14Z
dc.date.issued2009
dc.identifier.issn0377-0486
dc.identifier.issn1097-4555
dc.identifier.urihttps://doi.org/10.1002/jrs.2298
dc.identifier.urihttps://hdl.handle.net/20.500.12712/18389
dc.descriptionAYDIN, METIN/0000-0003-3767-946X; Canamares, Maria Vega/0000-0001-8900-3125en_US
dc.descriptionWOS: 000272521700014en_US
dc.description.abstractThe 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 (C-2h) 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 b(u) modes, along with somewhat weaker enhancement of the a(u) and b(g) modes. Copyright (C) 2009 John Wiley & Sons, Ltd.en_US
dc.description.sponsorshipNational Institute of Justice [2006-DN-BX-K034]; City University Collaborative Incentive program [80209]; National Science Foundation under Cooperative AgreementNational Science Foundation (NSF) [RII-9353488, CHE-0091362, CHE-0345987, ECS0217646]; City University of New York PSC-BHE Faculty Research Award Program.; National Science FoundationNational Science Foundation (NSF) [IMR 0526926]; National Natural Science Foundation of ChinaNational Natural Science Foundation of China [NSFC 20773045, 20627002]; Programme of Introducing Talent of Discipline to Universities [B06009]en_US
dc.description.sponsorshipWe are indebted to the National Institute of Justice (Department of Justice Award #2006-DN-BX-K034) and the City University Collaborative Incentive program (#80209). This work was further supported by the National Science Foundation under Cooperative Agreement No. RII-9353488, grant No. CHE-0091362, CHE-0345987 and grant number ECS0217646 and by the City University of New York PSC-BHE Faculty Research Award Program. We are also indebted to the National Science Foundation Grant # IMR 0526926, which supplied the Bruker Senterra/Ramanscope combined Dispersive Raman/FT Raman spectrometer. This work is also supported by the National Natural Science Foundation of China (NSFC 20773045 and 20627002) and the Programme of Introducing Talent of Discipline to Universities ('111' Project, B06009).en_US
dc.language.isoengen_US
dc.publisherWileyen_US
dc.relation.isversionof10.1002/jrs.2298en_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectFlavanthroneen_US
dc.subjectIndanthroneen_US
dc.subjectSERSen_US
dc.subjectDFTen_US
dc.titleSurface-enhanced Raman spectroscopy of indanthrone and flavanthroneen_US
dc.typearticleen_US
dc.contributor.departmentOMÜen_US
dc.identifier.volume40en_US
dc.identifier.issue11en_US
dc.identifier.startpage1557en_US
dc.identifier.endpage1563en_US
dc.relation.journalJournal of Raman Spectroscopyen_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US


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