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Utrera-Melero, R., Massuyeau, F., Latouche, C., Camerel, F. & Perruchas, S. (2022) Copper Iodide Clusters Coordinated by Emissive Cyanobiphenyl-Based Ligands. Inorg. Chem. 61 4080–4091. 
Added by: Richard Baschera (2022-06-02 13:20:18)   Last edited by: Richard Baschera (2022-06-02 13:56:33)
Type de référence: Article
DOI: 10.1021/acs.inorgchem.1c03876
Numéro d'identification (ISBN etc.): 0020-1669
Clé BibTeX: UtreraMelero2022
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Catégories: IMN, MIOPS
Créateurs: Camerel, Latouche, Massuyeau, Perruchas, Utrera-Melero
Collection: Inorg. Chem.
Consultations : 3/72
Indice de consultation : 10%
Indice de popularité : 2.5%
Liens URLs     https://doi.org/10 ... .inorgchem.1c03876
Résumé     
Copper(I) halides are currently the subject of intensive research because of their rich photophysical properties combined with economic and eco-friendly advantages for practical applications. The molecular copper iodide cluster of the general formula [Cu4I4L4] (L = ligand) is a well-known photoluminescent compound, and the possibility to enlarge the panel of its photophysical properties is studied here, by exploring ligands bearing a distinct emitter. The comparative study of five copper iodide clusters coordinated by different phosphine ligands functionalized by the emissive cyanobiphenyl (CBP) group is thus described in this work. The emissive properties of the ligands have a great impact onto the photophysical properties of the cluster. Compared with classical [Cu4I4L4] copper iodide clusters, the origin of the emission bands is largely modified. The CBP moiety of electron acceptor character significantly lowers in energy the vacant orbitals and consequently affects the global energetic layout. These clusters present dual emission based on two different emissive centers which interplay through energy transfer. This study demonstrates that the design of original ligands is an effective approach to enrich the photophysical properties of the appealing family of copper halide complexes.
  
Notes     
Publisher: American Chemical Society
  
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