The Journal of Physical Chemistry B
5. DISCUSSION AND CONCLUSION
Article
ASSOCIATED CONTENT
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S
* Supporting Information
The broad absorption and emission spectra of 1 contrast with
the narrow spectral features of 2. Narrow spectral features are,
in general, characteristic of squaraine dyes and are related to the
relatively small electron-vibration coupling in these systems
(small εν) and to the large mixing between the neutral and
zwitterionic states, typical of class II quadrupolar dyes,28 that
further reduces the effective vibrational coupling. Broad
absorption and fluorescence bands of 1 are instead typical of
largely neutral (class I) chromophores.28 These features hold
true also in the model discussed in this paper, accounting for
two independent reaction fields. The main spectroscopic
consequence of the presence of two reaction fields is
recognized in the sizable normal solvatochromism of linear
absorption spectra that cannot be rationalized in models
accounting for a single reaction field.
Essential-state models for nonlinear V-shaped quadrupolar
chromophores, like 1, have been recently discussed.32 The
appearance of a secondary band in the linear absorption
spectra, to the blue of the main band, marks the reduced
symmetry of bent molecules; the g → e transition, OPA-
forbidden and TPA-allowed in linear molecules, acquires a
sizable OPA intensity in bent molecules. This makes the overall
absorption spectrum of V-shaped quadrupolar chromophores
very broad; 1, a largely neutral chromophore, showing in the
green spectral region the typical broad absorption band of class
I dyes, shows an additional peak in the blue−violet region, due
to its V-shaped structure. The resulting absorption spectrum
then covers most of the solar spectrum, making this
chromophore, and more generally V-shaped quadrupolar
chromophores, promising for solar cell applications.
Figures S1−S3 show spectra calculated for the two compounds
with slightly different models. Figure S4 shows experimental
absorption spectra of chemical species mimicking the isolated
electron-acceptor and electron-donor groups. This material is
AUTHOR INFORMATION
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Corresponding Author
0521 905556.
Notes
The authors declare no competing financial interest.
ACKNOWLEDGMENTS
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This work was partly supported by the Indo−Italian Executive
Programme of Scientific and Technological Co-operation
2008−2010 and by Fondazione Cariparma through the Project
2010.0329. C.S. thanks the University of Parma and INSTM for
financial support. S.P. thanks the ISRO-IISc Space Technology
Cell for supporting this work through the Project ISTC/CSS/
STP/252, and S.R.B.K. thanks CSIR for a Senior Research
Fellowship.
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