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any spin polarization of the precursor is transferred to the
quinone. Therefore, the CA- resonance is expected to be in
absorption.
The time profile of the intensity of the CA- resonance was
analyzed in terms of formation and decay steps taking spin
polarization into account.7. The least-squares fit to the experi-
mental data is given by the solid line in Figure 8.
Table 2 summarizes rate constants and yields measured in
this work.
(8) Reference 2 and references therein.
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Flash photolysis and FT-EPR studies show that C60 triplets
are quenched by chloranil. FT-EPR spectra establish that
encounters between C60 and CA in benzonitrile leads to
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3
formation of CA- free radicals. The rate constant of the
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thermodynamic driving force. A comparison of 3C60 and CA-
resonance peaks shows that only about 20% of the quenching
events give cage escape products.
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In benzonitrile solutions of CA with Pe (or TTA) and C60,
excitation with visible light initiates a fast and efficient reduction
of CA. In the presence of Pe, the dominant reaction path is
3
3
formation of Pe by energy transfer from C60 followed by
oxidative quenching of 3Pe by CA. In this process the yield of
CA- compared to that of the direct excited state electron transfer
from C60 to CA is more than doubled. With the amine, reductive
3
quenching of C60 is followed by fast electron transfer from
C60- to CA. It is noteworthy that C60 catalyses electron-transfer
reactions that cannot be driven by visible light (TTA/CA) or
would be very inefficient because of low triplet quantum yield32
(Pe/CA). Since C60 absorbs light over a broad range of the
visible spectrum and has a triplet quantum yield close to one,
it may find application in solar-driven chemical reactions.
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Acknowledgment. We much appreciate financial support
for this work provided by the Division of Chemical Sciences,
Office of Basic Energy Sciences, of the U.S. Department of
Energy to the University of Massachusetts (DE-FG02-84ER-
13242) and to Brandeis University (DE-FG02-89ER14072).
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