Stellar Multi-Photon Absorption Materials: Beyond the Telecommunication Wavelength Band

dc.contributor.authorSchwich, Torsten
dc.contributor.authorBarlow, Adam
dc.contributor.authorCifuentes, Marie
dc.contributor.authorSzeremeta, J
dc.contributor.authorSamoc, Marek
dc.contributor.authorHumphrey, Mark
dc.date.accessioned2020-12-20T20:57:53Z
dc.date.available2020-12-20T20:57:53Z
dc.date.issued2017
dc.date.updated2020-11-23T11:10:28Z
dc.description.abstractVery large molecular two- and three-photon absorption cross-sections are achieved by appending ligated bis(diphosphine)ruthenium units to oligo(p-phenyleneethynylene) (OPE)-based “stars” with arms up to 7 phenyleneethynylene (PE) units in length. Extremely large three- and four-photon absorption cross-sections, through the telecommunications wavelengths range and beyond, are obtained for these complexes upon optimizing OPE length and the ruthenium-coordinated peripheral ligand. Multi-photon absorption (MPA) cross-sections are optimized with stars possessing arms 2 PE units in length. Peripheral ligand variation modifies MPA merit and, in particular, 4-nitrophenylethynyl ligand incorporation enhances maximal MPA values and “switches on” four-photon absorption (4PA) in these low molecular-weight complexes. The 4-nitrophenylethynyl-ligated 2PE-armed star possesses a maximal four-photon absorption cross-section of 1.8×10−108 cm8 s3 at 1750 nm, and significant MPA activity extending beyond 2000 nm
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0947-6539
dc.identifier.urihttp://hdl.handle.net/1885/218414
dc.language.isoen_AUen_AU
dc.publisherWiley-VCH Verlag GMBH
dc.sourceChemistry, A European Journal
dc.titleStellar Multi-Photon Absorption Materials: Beyond the Telecommunication Wavelength Band
dc.typeJournal article
dcterms.accessRightsOpen Access
local.bibliographicCitation.issue35
local.bibliographicCitation.lastpage8399
local.bibliographicCitation.startpage8395
local.contributor.affiliationSchwich, Torsten, College of Science, ANU
local.contributor.affiliationBarlow, Adam, College of Science, ANU
local.contributor.affiliationCifuentes, Marie, College of Science, ANU
local.contributor.affiliationSzeremeta, J, Wroclaw University of Technology
local.contributor.affiliationSamoc, Marek, Wroclaw University of Technology
local.contributor.affiliationHumphrey, Mark, College of Science, ANU
local.contributor.authoremailu9410034@anu.edu.au
local.contributor.authoruidSchwich, Torsten, u4450603
local.contributor.authoruidBarlow, Adam, u4125124
local.contributor.authoruidCifuentes, Marie, u9410034
local.contributor.authoruidHumphrey, Mark, u9400918
local.description.notesImported from ARIES
local.identifier.absfor020503 - Nonlinear Optics and Spectroscopy
local.identifier.ariespublicationu5378827xPUB21
local.identifier.citationvolume23
local.identifier.doi10.1002/chem.201702039
local.identifier.scopusID2-s2.0-85020064899
local.identifier.thomsonID000404009500012
local.identifier.uidSubmittedByu5378827
local.type.statusAccepted Version

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