consequence of bridging ligand design, which slows down
intercomponent energy transfer. By contrast, energy transfer is
effective at 77 K, because of the long intrinsic excited-state lifetime
of the donor chromophore(s) under these experimental conditions.
This work was supported by PRIN 2003. Project title:
‘‘Molecular devices for the harvesting, conversion and storage of
light energy’’, FISR, project title ‘‘Nanotecnologie molecolari per
l9immagazzinamento e la trasmissione delle informazioni’’ and
FIRB, project no. RBNE019H9K.
Notes and references
Fig. 4 Structural formulae of compounds 4 and 5.
{ Selected data for ligand L. Isolated yield: 70%. 1H-NMR (CDCl3,
300MHz) d 8.84 (s, 4H), 8.78 (m, 4H), 8.72 (d, 4H, J 5 12.0 Hz), 8.05 (d,
4H, J 5 12.5 Hz), 7.92 (ddd, 4H, J 5 2.8, 8.8, 12.0 Hz), 7.84 (d, 4H,
J 5 12.5 Hz), 7.80 (bs, 1H), 7.54 (bs, 2H), 7.36–7.41 (m, 4H), 2.55 (s, 3H).
13C-NMR (CDCl3, 75MHz) d 149.2, 136.8, 127.7, 127.3, 123.8, 123.5,
121.4, 118.7, 21.5. ES-MS (MeOH/CH3COOH): m/z (%) 5 707.0 (100).
Anal. Calcd. for C49H34N6: C, 83.26; H, 4.85; N, 11.89. Found: C, 83.20;
H, 4.88; N, 11.80%. Selected data for [(terpy)Ir(L)Ru(L)Ru(L)-
absorb at wavelength longer than 480 nm. On the basis of the
lifetimes of the 570 nm emission of 2 and 3, energy transfer from
3
the higher-lying MLCT/3LC emitting state of the Ir(III) subunits
3
to the lower-lying MLCT levels of the Ru(II) components is not
effective in 3 at room temperature. The inefficiency of the energy
transfer indicates that such a process should be significantly slower
than the room temperature intrinsic decay rate of 2, that is 3.7 6
105 s21, in spite of the non-negligible driving force (about 0.3 eV,
from emission data). Electronic factors have to be at the origin of
such a behavior. Energy transfer between Ru(II) and Os(II)
polypyridine subunits having three interposed phenyls
(compound 4 in Fig. 4) is reported to occur with a rate constant
of 6.7 6 108 s21, by a Dexter mechanism (superexchange),12 in
spite of the low electronic interaction energy Hen, which was
calculated to be lower than 1 cm21 (driving force is comparable to
that of 3). In a similar Ru(II)/Rh(III) species (5, Fig. 4),
photoinduced *Ru-to-Rh electron transfer takes place with a rate
1
Ir(terpy)](PF6)10 (3). Isolated yield: 15%. H-NMR (CD3CN, 300MHz) d
9.12 (s, 12H), 8.73 (bd, 14H, J 5 8.2 Hz), 8.40 (bd, 16H, J 5 8.2 Hz), 8.21
(bd, 18H, J 5 8.2 Hz), 8.10 (bs, 3H), 7.99 (m, 16H, J 5 7.8 Hz), 7.81 (s,
6H), 7.51 (m, 16H), 7.24 (m, 14H), 2.65 (s, 9H). 13C-NMR (CDCl3,
75MHz) d 159.1, 156.4, 153.3, 148.6, 143.6, 141.4, 140.7, 138.9, 136.8,
130.7, 130.0, 129.2, 128.6, 125.4, 124.0, 122.4, 21.6. Anal. Calcd. For
C177H124F60Ir2N24P10Ru2: C, 45.98; H, 2.70; N, 7.27. Found: C, 46.20; H,
2.90; N, 7.20%.
1 V. Balzani, A. Credi and M. Venturi, Molecular Devices and Machines,
Wiley-VCH, Weinheim, 2003, ch. 2–6 and references therein.
2 See, for example: (a) V. Balzani, S. Campagna, G. Denti, A. Juris,
S. Serroni and M. Venturi, Acc. Chem. Res., 1998, 31, 26; (b)
M. H. V. Huynha, D. M. Dattelbauma and T. J. Meyer, Coord. Chem.
Rev., 2005, 249, 457.
3 P. Coppo, M. Duati, V. N. Kozhevnikov, J. W. Hofstrat and L. De Cola,
Angew. Chem., Int. Ed., 2005, 44, 1806.
4 (a) B. W. D_ Andrade and S. R. Forrest, Adv. Mater., 2004, 16, 1585;
(b) J. Slinker, D. Bernerds, P. L. Houston, H. D. Abruna, S. Bernhard
and G. G. Malliaras, Chem. Commun., 2003, 2392.
5 (a) A. Juris, V. Balzani, F. Barigelletti, S. Campagna, P. Belser and
A. von Zelewsky, Coord. Chem. Rev., 1988, 84, 85; (b) T. J. Meyer, Pure
Appl. Chem., 1986, 58, 1193; (c) G. A. Crosby, J. Chem. Educ., 1983, 60,
791.
6 I. M. Dixon, J.-P. Collin, J.-P. Sauvage, L. Flamigni, S. Encinas and
F. Barigelletti, Chem. Soc. Rev., 2000, 29, 385 and references therein.
7 V. Balzani, A. Juris, M. Venturi, S. Campagna and S. Serroni, Chem.
Rev., 1996, 96, 759 and references therein.
8 (a) C. J. Aspley and J. A. G. Williams, New J. Chem., 2001, 25, 1136; (b)
W. Goodall, K. Wild, K. J. Arm and J. A. G. Williams, J. Chem. Soc.,
Perkin Trans. 2, 2002, 1669.
9 J.-P. Collin, I. M. Dixon, J.-P. Sauvage, J. A. G. Williams, F. Barigelletti
and L. Flamigni, J. Am. Chem. Soc., 1999, 121, 5009.
10 (a) G. R. Newkome, T. J. Cho, C. N. Moorefield, R. Cush, P.S. Russo,
L. A. God´ınez, M. J. Saunders and P. Mohapatra, Chem. Eur. J., 2002,
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and L. A. God´ınez, Chem. Eur. J., 2002, 10, 1493.
11 (a) E. Baranoff, I. M. Dixon, J.-P. Collin, J.-P. Sauvage, B. Ventura and
L. Flamigni, Inorg. Chem., 2004, 43, 3057; (b) L. Flamigni, B. Ventura,
F. Barigelletti, E. Baranoff, J.-P. Collin and J.-P. Sauvage, Eur. J. Inorg.
Chem, 2005, 1312.
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Chem. Soc., 1999, 121, 4207.
13 F. Scandola, C. Chiorboli, M. T. Indelli and M. A. Rampi, in Electron
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vol. 3, p. 337.
constant of 3.0 6 107 s21 13
However, the introduction of hexyl
.
substituents on the central phenyl ring of this latter species
decreases the electron transfer rate constant to 1.1 6 106 s21, as a
consequence of a decrease in the adjacent coupling terms of the
superexchange mechanism, due to variation in the twist angle
between the phenyl rings. The examples mentioned deal with para-
polyphenyls: in our system, a meta arrangement is present, and this
should affect the electronic interactions to a much larger extent
than the presence of ring substituents. Therefore, a significantly
lower Hen for the energy transfer in 3 compared to 4 is expected,
which would translate into an intercomponent energy transfer rate
slower than 105 s21, as suggested by the observed results.
At 77 K, energy transfer from Ir-based to Ru-based chromo-
phores is quantitative, as the only emission recorded is the
Ru-based 3MLCT emission regardless of the excitation wavelength
(Fig. 3, Table 1). Under these conditions, the excited-state lifetime
of the Ir(III) subunit(s) is quite long (205 ms) thus allowing the
energy transfer pathway to successfully compete with the intrinsic
decay of the Ir(III) centers. Indirectly, the room and low
temperature results tend to suggest that Ir-to-Ru energy transfer
in 3 (a process which is expected to be less sensitive to temperature)
would occur with a rate constant of the order of 104 s21
.
In summary, we have prepared a tetranuclear, mixed-metal
multichomophoric species capable of exhibiting two-colors, almost
independent emission at room temperature: this feature is a
5268 | Chem. Commun., 2005, 5266–5268
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