| Literature DB >> 31794079 |
Thomas Brandl1, Christoph Kerzig1, Loïc Le Pleux1, Alessandro Prescimone1, Oliver S Wenger1, Marcel Mayor1,2,3.
Abstract
The development of molecular materials for conversion of solar energy into electricity and fuels is one of the most active research areas, in which the light absorber plays a key role. While copper(I)-bis(diimine) complexes [CuI (L)2 ]+ are considered as potent substitutes for [RuII (bpy)3 ]2+ , they exhibit limited structural integrity as ligand loss by substitution can occur. In this article, we present a new concept to stabilize copper bis(phenanthroline) complexes by macrocyclization of the ligands which are preorganized around the CuI ion. Using oxidative Hay acetylene homocoupling conditions, several CuI complexes with varying bridge length were prepared and analyzed. Absorption and emission properties are assessed; rewardingly, the envisioned approach was successful since the flexible 1,4-butadiyl-bridged complex does show enhanced MLCT absorption and emission, as well as improved photostability upon irradiation with a blue LED compared to a reference complex.Entities:
Keywords: copper complexes; ligand design; macrocycles; photochemistry; photostability
Year: 2020 PMID: 31794079 PMCID: PMC7079024 DOI: 10.1002/chem.201904754
Source DB: PubMed Journal: Chemistry ISSN: 0947-6539 Impact factor: 5.236
Figure 1Concept to stabilize the ligand sphere by interlinking both phenanthroline ligands to a tetradentate macrocycle. To allow the macrocyclic ligand to adapt to the requirements imposed by the CuI coordination sphere, the rigid diacetylene bridges were hydrogenated to the corresponding saturated buta‐1,4‐diyl bridges in the case of target compound 1.
Scheme 1Synthesis of the copper complexes 1 and 2: a) 8, K2CO3, Pd(PPh3)4, toluene/H2O (6:1), reflux, 20 h, 52 %; b) [Cu(MeCN)4][PF6], DCM, RT, 30 min, quant.; c) K2CO3, DCM/MeOH (1:1), RT, 12 h, quant.; d) CuCl, TMEDA, DCM, RT, 5 h, quant.; e) 9, tBuXPhos, K3PO4, Pd(OAc)2, toluene, reflux, 12 h, 72 %; f) TBAF, THF, RT, 10 min, 99 %; g) TMSCl, nBuLi, THF, −78 °C, 30 min, 68 %; h) [Cu(MeCN)4][PF6], DCM, RT, 30 min, quant.; i) CuCl, TMEDA, K2CO3, DCM/MeOH (1:1), RT, 1 h, 79 %; j) H2, Pd/C, MeOH, reflux, 20 h, 48 %.
Figure 2Solid‐state structure of 11 with rotation ellipsoids at 50 % probability. Hydrogen atoms and the PF6 − counterion were omitted for clarity. Color code: N: blue, Cu: yellow. The carbon atoms are colored purple and grey to differentiate both ligand systems optically. The angle between the phenanthrolines was measured to be 60.15° and Cu−N bond lengths were measured to be between 2.026 and 2.117 Å. CCDC https://www.ccdc.cam.ac.uk/services/structures?id=doi:10.1002/chem.201904754 contains the supplementary crystallographic data for this paper. These data are provided free of charge by http://www.ccdc.cam.ac.uk/.
Scheme 2Synthesis of the reference CuI complex 15: a) tBuXPhos, K3PO4, Pd(OAc)2, toluene, reflux, 12 h, 68 %; b) Cu(MeCN)4⋅PF6, DCM, RT, 30 min, quant.
Figure 3UV/Vis spectra of the macrocyclic complex 1 and the reference complex 15 measured in acetonitrile at room temperature. To improve their visibility, the MLCT absorption bands in the visible were increased by the indicated scaling factors.
UV/Vis absorption maxima and extinction coefficients of 1, 15, and [Cu(Me2phen)2[PF6].
|
Compd. |
|
|
|---|---|---|
|
|
292 (39 510) |
452 (2740) |
|
|
287 (42 690) |
433 (580) |
|
[Cu(Me2phen)2][PF6] |
273 (45 000) |
456 (5900) |
Figure 4a) DFT‐optimized structure of 1 at the B3LYP/LANL2DZ level of theory displaying the computed HOMO (left) and LUMO (right) orbitals. Comparison of computed ground‐state (left) and excited‐state geometries (right) of b) the macrocyclic complex 1 and c) the reference complex 15 (bottom). The angles measured between both phenanthroline planes are given in ruby red.
Figure 5Emission spectrum of complex 1 in frozen CH3CN matrix at 77 K after excitation at 532 nm with laser pulses of ≈10 ns duration. The spectrum was time‐integrated over 100 ns starting with the laser pulse (pulse energy, 30 mJ). The sharp peak at 532 nm is due to stray excitation light.
Figure 6a) UV/Vis data of 1 (top) and 15 (bottom) recorded after different periods of LED illumination (455 nm, 500 mW optical output) to investigate photostability. b) Development of the absorption of 15 at 433 nm during the experiment.