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of DTPA and TTPA, and it shows that the melting temperatures
of DTPA and TTPA are 162 1C and 113 1C, respectively. The above
results indicate that the melting temperature of TTPA is much
less than that of DTPA, due to the presence of the increased
number of alkoxy chains at the periphery. In addition to that,
there is no glass transition temperature detected; the reason for
that may be that the structures of DTPA and TTPA are too rigid.
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To summarize, novel triphenylamine-based star-like molecules
have been synthesized and well characterised using various
spectral data. The photophysical properties of the newly synthesized
star-like molecules of DTPA and TTPA were carried out in various
solvents. Comparing the two compounds DTPA and TTPA, both the
compounds have similar photo behaviours and almost equal life-
times in the excited state. This may be due to inter-branch coupling,
as a result of cooperative enhancement. Furthermore, the two newly
synthesized molecules exhibit a broad absorption range cover-
ing the whole visible spectral region in solution as well as in the
solid thin film phase. Based on the thermogravimetric results,
DTPA is more stable than TTPA. Hence, these photophysical
and electrochemical properties highlight that these materials
are potential candidates for use as donor materials in solution-
processable organic photovoltaic cells.
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Acknowledgements
RB and AS acknowledge the financial support of the Department
of Science and Technology, New Delhi, India (Grant No. SR/F/
1584/2012-13), Council of Scientific and Industrial Research,
New Delhi, India (Grant No. 01(2540)/11/EMR-II) and University
Grants Commission, New Delhi, India (Grant No. UGC No.41-
215/2012 (SR). VT thanks UGC-FRP (Grant No. F. 4-5(24-FRP)/
2013(BSR)) for financial support.
´
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