Dalton Transactions
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band (16 to 35 nm). This can be an indicator of dipolar elec-
tronic transitions.10 The Stark-derived Σβ0 values for the series
(Table 3, see ESI† for details of fitting and extraction of charge
transfer parameters) follow a similar trend to HRS β0, although
measurement and fitting uncertainties are large and in all
cases values are larger than HRS β0 – a common observation in
prior work.5b,7,11 Similar to 3, the fit of the main low energy
peak in 2 consists of three Gaussians, each at slightly higher
energy than those of 3. Dipole moment changes Δµ and
charge transfer distances r associated with these peaks in 2
and 3 are within experimental error of one another (though
consistently slightly higher for 2), as are most other measured
parameters. However, an additional peak in 2 requires a 4th
Gaussian for an adequate fit, and while its transition is less
dipolar in nature (lower Δµ values) it shows strong electronic
coupling (higher Hab) and a high value of µ12 means that it
contributes significantly to Σβ0. In 1, the four Gaussian com-
ponents have less dipolar character their counterparts in 1 and
3, and generally electronic coupling is stronger than in either 2
or 3. The overall picture suggests that 2 hits a sweet spot where
transitions are just as dipolar than those of 3, yet electronic
communication across the diphenylacetylene bridge is strong.
TD-DFT calculations of the electronic spectra and β values
of 1 to 3 in acetonitrile solvent have been performed using the
ADF program, with the SAOP functional and TZ2P basis set.
Previously,5b we showed that a solvent forcefield is necessary
for these calculations to reflect experimental trends, although
the β-values computed were much larger (up to 30×) than
those observed experimentally. The methods used here are an
incremental improvement on those previously published.
Values are closer to experiment, but still high (reflecting low
computed transition energies, see ESI†), and the trend is an
excellent match for Stark and HRS findings. βzzz, 0 of 960 (1),
1300 (3) and 2160 × 10−30 (2) are obtained, and normalising all
three techniques to 2 as 100% (Table S2†) makes it clear just
how good the agreement in trend is between experiment and
theory. A qualitative interpretation of the TD-DFT-computed
orbital-to-orbital transitions is thus justified, and reveals two
key differences between 2 and 3. Firstly, the HOMO level of 2 is
concentrated on the NPh2 group and immediately appended
aryl ring (Fig. 4), whereas in 3 it spreads across the entire
organic system – as does the HOMO−1 for both systems. This
may increase the dipole moment change associated with
strong, low energy transitions to the LUMO+6 and LUMO+8,
which spread across POM and imido-ring, and is reflected in
the very slightly higher Δµ values found for 2 by Stark
(although they are within experimental error of those for 3).
Secondly, 3 has a weak transition from an imido-phenyl based
HOMO−5, to a POM-based LUMO+7, at a high computed
energy (3.39 eV, Table S5 and Fig. S7†). In 2, a similar tran-
sition is observed from the HOMO−9 to LUMO+1 (Table S4
and Fig. S6†), but the calculated energy is 0.7 eV lower and cal-
culated fos nearly 3× higher – possibly due to involvement of
the alkyne bridge. This seems consistent with the fourth
Gaussian peak used to fit the Stark spectrum of 2, which has
both moderately high Hab and Δμ, and appears responsible for
Fig. 3 (a) ORTEP representation of the molecular anions in 1 and 2.
Disordered parts omitted for clarity, thermal ellipsoids are at the 30%
probability level, C atoms are grey; Mo, green; O, red; N, blue. H atoms
are white spheres of arbitrary radii. (b) Crystal packing in 2 viewed along
the crystallographic a-axis. For clarity, NBu4 cations are colored blue
and [Mo6O18NPhCCPhNPh2]2− anions are colored green.
+
2 this is only ca. 22°, and in 1 19°. Moreover, the imido (accep-
tor) ring in 2 shows a shortening of the ortho-to-meta C–C
bonds (mean distance 1.36(2) Å vs. 1.42(2) Å for ortho/meta-to-
para), suggesting a significant contribution from a quinoidal
resonance form. This is not present in the imido ring of 3,
while in 1 disorder and application of various restraints pre-
cludes such in depth analysis. However, it should be noted the
weak rotational barrier of unhindered phenylacetylenes (ca.
1 kcal mol−1)9 means that these differences will not persist in
solution. The X-ray structure of 2 also reveals that it is the first
POMophore to crystallize in a non-centrosymmetric space
group (Pna21), with polar packing of chromophore dipoles.
These are oriented at ca. 90° to one another, giving the struc-
ture net polarity (Fig. 4b) and making it a potential bulk NLO
material. Instability resulting from large solvent occupied void
spaces has prevented further investigation of this, but the
result suggests that adding steric bulk to the organic system
may be one way to counteract the influence of the POM in the
crystallization process and encourage formation of polar
materials.
Evidence that differences in electronic structure between 1,
2 and 3 persist in glasses and solution is provided by a combi-
nation of Stark spectroscopy (see ESI† for details), and DFT
calculations. In Stark, the low temperature (77 K) electronic
absorption spectra in butyronitrile have a similar overall form
to the room temperature spectra in MeCN, but all three com-
pounds show substantial red shifts in the low-energy IHCT
Fig. 4 TDF-DFT calculated HOMOs for 1 to 3 (bottom) and most
important acceptor orbitals LUMO+x (in terms of oscillator strength
(top)).
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Dalton Trans.