ChemComm
Communication
Table 1 Relative energy, absorption and emission properties of KK and EE
tautomers of DH, DM and DA computed at the B3LYP/6-31+g* level
of theory
DMEE and DAEE are 507, 521 and 527 nm, respectively, and
can be compared to the experimental emission maximum of
560 nm for DAEE (Table 1). Clearly, the DFT calculations
reiterate that the appearance of the new red shifted peak is
due to the formation of the enolic tautomer.
Molecule
Tautomer
DH
KK
DM
KK
DA
KK
EE
EE
EE
The relative energies (Table 1) of the EE minima in the S1 state
revealed that DHEE and DMEE are B29 kcal molÀ1 higher than that
of the KK form, whereas only B20 kcal molÀ1 for DAEE. The
additional stabilization of B10 kcal molÀ1 seen in DAEE clearly
demonstrates that the KK to EE tautomerization of DA in the S1
state is energetically more favorable compared to that of DH and
DM systems. Although the tautomerization barrier in the S1 state
could not be calculated, it can be expected that such stabilization of
the transition state connecting the KK and EE forms may be seen
for DA. The above results explain the appearance of a new red
shifted absorption due to enol formation and the importance of
aryl substitution to enable keto–enol tautomerization in the excited
state, a phenomenon not seen for other derivatives. The complete
photophysical processes during irradiation of DH and DA systems
Relative energy (kcal molÀ1
)
S0
S1
0.0
0.0
34.0
28.5
0.0
0.0
34.0
27.6
0.0
0.0
35.9
20.0
Vertical excitation wavelength (nm)
S1
S2
S3
316
316
293
318
309
306
316
316
295
319
310
306
318
318
302
345
330
327
a
labs
—
—
o250
—
300
390
Emission wavelength (nm)
lem
lem
386
—
507
—
385
—
521
—
386
—
327
560
b
a
Experimental absorption maximum. b Experimental emission maximum.
emission wavelengths may not match with the experiments owing to are given in Fig. S14 (ESI†) for comparison.
the gas-phase nature of the calculations, qualitative and important
To summarize, we have demonstrated the photoenolization
insight into the experimental observations can be deduced from of DA, via ESDPT. To the best of our knowledge, this is the first
the DFT results. The ground and excited state minimum energy report on light triggered enolization of a dipyrromethane
structures of DAEE showed distinct differences in the orientation of derivative with ‘‘turn on’’ fluorescence and emissive even in
the aryl and pyrrole rings (Fig. S12, ESI†). The relative energy the solid state. DFT calculations confirm the importance of the
calculations showed that in the ground state, the DAEE, DMEE and diaryl group at the meso-carbon that stabilizes the dienol form
DHEE are B34.0 kcal molÀ1 higher in energy than the KK forms in the excited state compared to monoaryl or dimethyl groups.
irrespective of the meso-carbon substitution (Table 1).
The computed excitation energies and the molecular orbitals shifted emission of the molecule as sensors will be explored.
contributing to the excitations are given in Table 1 and Fig. S13 KCGS, APT and RP thank CSIR, New Delhi, for fellowship.
In future, the application of the light triggered large Stokes-
(ESI†) respectively. It can be seen that for DAKK, the transitions We thank Dr Arun Kumar, NISER, for X-ray structure of DA.
resulted from charge redistribution in the pyrrole rings, whereas
in DAEE, there is an extension of conjugation from pyrrole to the
phenyl ring. For all the three KK structures, the S1 and S2 states
Notes and references
1 (a) Y. Sagara and T. Kato, Nat. Chem., 2009, 1, 605; (b) H. Maeda,
are due to n–p* (HOMO À 6 to LUMO, HOMO À 6 to LUMO + 1,
Y. Bando, K. Shimomura, I. Yamada, M. Naito, K. Nobusawa,
H. Tsumatori and T. Kawai, J. Am. Chem. Soc., 2011, 133, 9266.
respectievely) transitions and are degenerate, while S3 is due to
p–p* (HOMO to LUMO) transition. In the case of EE structures,
all the first three excited states are p–p* [HOMO to LUMO (S1),
HOMO À 1 to LUMO (S2), and HOMO À 1 to LUMO + 1 (S3)] in
nature and the S2 and S3 states are nearly degenerate. The
2 (a) G. Mayer and A. Heckel, Angew. Chem., Int. Ed., 2006, 45, 4900;
(b) Q. Chen, D. Zhang, G. Zhang, X. Yang, Y. Feng, Q. Fan and D. Zhu,
Adv. Funct. Mater., 2010, 20, 3244; (c) T. Kobayashi, T. Komatsu,
´
´
M. Kamiya, C. Campos, M. Gonzalez-Gaitan, T. Terai, K. Hanaoka,
T. Nagano and Y. Urano, J. Am. Chem. Soc., 2012, 134, 11153.
3 (a) D. R. Morris and L. P. Hager, J. Biol. Chem., 1966, 241, 3582;
(b) A. Taurog, Endocrinology, 1976, 98, 1031; (c) S. A. Aziz and
C. O. Knowles, Nature, 1973, 242, 417–418.
vertical excitation energies are similar (316–293 nm) for DHKK
,
DMKK, and DAKK, again showing the absence of substituent
effects in the excited states of the KK forms (Table 1). The enols,
DHEE and DMEE also showed similar absorption energies
(319–306 nm) and interestingly these are also similar to those
of the KK forms. However, DAEE showed a red shift of 43 nm
4 (a) H. Fischer and W. Gleim, Justus Liebigs Ann. Chem., 1935, 521, 157;
(b) A. Wiehe, C. Ryppa and M. O. Senge, Org. Lett., 2002, 4, 3807.
5 N. Kumar, S. Chakravorti and P. Chowdhury, J. Mol. Struct., 2008,
891, 351.
6 K. C. G. Sreedevi, A. P. Thomas, P. S. Salini, S. Ramakrishnan,
K. S. Anju, M. G. D. Holaday, M. L. P. Reddy, C. H. Suresh and
A. Srinivasan, Tetrahedron Lett., 2011, 52, 5995.
(l = 345 nm) compared to that of the p–p* (S3) state of DAKK
.
The red shift in the vertical absorption wavelength seen in
DAEE is consistent with the experimental observation and can
be attributed to the extended charge delocalization seen in the
p-orbitals of the pyrrole and the aryl rings that are involved in
the transitions in DAEE. The emission energies of the KK forms
of all the three molecules are similar (B386 nm) indicating that
there is little effect of the substituents on their emission
7 R. Deans, J. Kim, M. R. Machacek and T. M. Swager, J. Am. Chem.
Soc., 2000, 122, 8565.
8 (a) C. A. Rice, I. Dauster and M. A. Suhm, J. Chem. Phys., 2007,
126, 134313; (b) B. M. Giuliano, I. Reva and R. Fausto, J. Phys. Chem.
A, 2010, 114, 2506.
9 Y. Chiang, A. J. Kresge, Q. Meng, R. A. More O’Ferrall and Y. Zhu,
J. Am. Chem. Soc., 2001, 123, 11562.
10 (a) A. D. Becke, J. Chem. Phys., 1993, 98, 5648; (b) P. J. Stephens,
F. J. Devlin, C. F. Chablowski and M. J. Frisch, J. Phys. Chem., 1994,
98, 11623; (c) R. H. Hertwig and W. Koch, Chem. Phys. Lett., 1997, 268, 345.
properties. The emission wavelengths calculated for DHEE
,
This journal is ©The Royal Society of Chemistry 2014
Chem. Commun., 2014, 50, 8667--8669 | 8669