We
report the syntheses, structures, and luminescence properties of a
series of copper-iodo cuboids supported by L-type antimony ligands.
The cuboids are of general formula [(SbR3)4Cu4(I)4] (1–4, 8), where SbR3 is a series of homoleptic and heteroleptic
stibines containing both phenyl and a variety of alkyl substituents
(R = Cy,
i
Pr,
t
Bu, Ph); triphenyl,
i
Pr2Ph,
and Me2Ph stibines resulted in the formation of dimers
of type [(SbR3)4(Cu)2(I)2] (5–7). While similar luminescent
copper-halide cubes have been studied, the corresponding “heavy-atom”
congeners have not been studied, and ligation of such heavy-atom moieties
is often associated with long-lived triplet states and low-energy
absorption and emission profiles. Overall, two obligate parameters
are found to imbue NIR emission: (i) short Cu–Cu
bonds and (ii) high crystallographic symmetry; both
of these properties are found only in [(Sb
i
Pr3)4Cu4(I)4] (1, in I23; λem = 711 nm).
The correlation between NIR emission and high crystallographic symmetry
(which intrinsically includes high molecular symmetry)–versus only molecular symmetry–is confirmed by the counterexample
of the molecularly symmetric
t
Bu-substituted cuboid [(Sb
t
Bu3)4Cu4(I)4] (3, λem = 588 nm, in R-3), which
crystallizes in the lower symmetry trigonal space group. Despite the
indication that the stronger donor strength of the Sb
t
Bu3 ligand should red-shift emission beyond
that of the Sb
i
Pr3-supported
cuboid, the emission of 3 is limited to the visible region.
To further demonstrate the connection between structural parameters
and emission intensity, X-ray structures for 1 and 3 were collected between 100 and 300 K. Lastly, DFT calculations
for 1 on its singlet (S0) and excited triplet
state (T1) demonstrate two key factors necessary for low-energy
NIR emission: (i) a significant contraction of the
interconnected Cu4 intermetallic contacts [∼2.45
→ 2.35 Å] and (ii) highly delocalized
(and therefore low-energy) A
1 symmetry
HOMO/LUMO orbitals from which the emission occurs. Thus, any molecular
or crystallographic distortion of the Cu4 core precludes
the formation of highly symmetric (and low-energy) HOMO/LUMO orbitals
in T1, thereby inhibiting low-energy NIR emission.