C O M M U N I C A T I O N S
indicates that electrocyclic ring closure of singlet 3 and ring opening
of singlet 3a occur via a pericyclic funnel with small or nonexistent
barriers.13 Entry to this funnel from singlet 3 results in formation
of 4 with a quantum yield of 0.64, providing an upper bound of
0.36 for the quantum yield of return to the ground state of 3 via
the pericyclic funnel.
The thermal sigmatropic hydrogen shift of 3a also has a low
inherent barrier. In fact, 3a can be detected by means of steady-
state irradiation only at low temperatures and high solvent viscosi-
ties. A barrier of e2 kcal/mol for the hydrogen-shift reaction
appears to be consistent both with our data and with the laser flash
photolysis data of Lapouyade et al.4 for the R-phenyl analogue of
1. This barrier is substantially lower than the value of 41 kcal/mol
reported for the sigmatropic hydrogen shift of 1,3-cyclohexadiene.14
It also lower than the lowest barrier reported to date for a
sigmatropic hydrogen shift, the conversion of isoindene to indene
(ca. 14 kcal/mol).15 The low barrier for the rearrangement of 3a to
4 is, no doubt, a consequence of the highly exergonic nature of
this process.
Figure 2. UV spectra of irradiated 2 × 10-5 M 2-vinyl-1,3-terphenyl (3)
in methylcyclohexane at 77 K (time in minutes) and the calculated UV
spectrum of intermediate 3a.
In summary, molecular symmetry confines 3 to a single ground-
state conformation in which the vinyl and an o-phenyl group have
a syn relationship favorable for photocyclization. Cyclization yields
the intermediate 3a, the first 8a,9-dihydrophenanthrene to be directly
observed under steady-state irradiation conditions. Irradiation of
3a at 500 nm results in reversion to 3, whereas warming of the
glass or irradiation of 3 in fluid solution results in formation of 4.
Both the photochemical and thermal rearrangements are remarkable
for their low activation energies. Further details of this and related
reactions are under investigation.
The photochemical behavior of 1 can be readily explained with
reference to Scheme 1. The long-lived fluorescence is assigned to
the major (99%) rotamer, anti-1, which has a florescence quantum
yield and decay time similar to those of 1-phenylpropene.10 The
photocyclization of 1 to yield 2 is attributed to the minor (1%)
rotamer, syn-1. The absence of spectral changes upon irradiation
of 1 at 77 K is attributed to the very low population of syn-1 at
low temperature. The photochemical behavior of 3 can be explained
with reference to Scheme 2. The ground-state energies in Scheme
Scheme 2. Potential Energy Surfaces for the Photoreaction of
2-Vinyl-1,3-terphenyl (3) (Energies in eV)
Acknowledgment. Funding for this project was provided by
NSF Grants CHE-0100596 (F.D.L.) and CHE-0096889 (V.G.). We
thank Professor I. Alabugin, Florida State University, for calculating
the spectrum of 3a and for helpful suggestions.
References
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(2) The tandem photocyclization of several styrylfurans under anerobic
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2 have been estimated using MM/PM3 calculations, and the excited-
singlet-state energies, using ZINDO calculations for 3 and 4 and a
TD-DFT calculation for 3a.9,11 The absence of fluorescence from
3 both at room temperature and 77 K, the high quantum yield for
formation of 4 at room temperature, and the formation of 3a in a
rigid MC glass at 77 K are all indicative of a low barrier for
photocyclization. In this respect, the photocyclization behavior of
singlet 3 is similar to that of cis-stilbene, for which a barrier of e1
kcal/mol has been estimated for formation of 4a,4b-dihydrophenan-
threne.12 The singlet energy of 3 lies well above that of 3a, making
adiabatic conversion of 13* to 13a* energetically feasible. However,
the observation that irradiation of 3a yields 3 even in a 77 K glass
(9) TD-DFT calculations provided by I. Alabugin.
(10) Lewis, F. D.; Bassani, D. M.; Caldwell, R. A.; Unett, D. J. J. Am. Chem.
Soc. 1994, 116, 10477-10485.
(11) ZINDO calculations: CAChe, version 4.4; Oxford Molecular Group,
Inc.: Campbell, CA, 2000. Similar values of the singlet state energies of
3a (4.25 eV) and 4 (4.08 eV) can be estimated from their absorption and
fluorescence spectra, respectively.
(12) (a) Saltiel, J.; Waller, A. S.; Sears, D. F. J. J. Am. Chem. Soc. 1993, 115,
2453-2465. (b) Muszkat, K. A. Top. Curr. Chem. 1980, 88, 89-143.
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