3414 J. Phys. Chem. A, Vol. 108, No. 16, 2004
Tranter et al.
route to the total fulvene concentration will have to be
determined from detailed modeling.
Eight stable C6H6 isomers have been positively identified in
this work, including the important observation for the first time
of cis-1,3-hexadiene-5-yne and trans-1,3-hexadiene-5-yne. These
two species and their appearance temperatures conclusively
demonstrate the existence of a low-temperature route to benzene
that does not require the formation and subsequent isomerization
of fulvene. Thus, for the lower temperatures in this work, fulvene
and benzene are formed simultaneously by separate reaction
paths. Recent theoretical analyses of the likely reaction paths
appear to be completely consistent with this observation.
Furthermore, 1,2-hexadiene-5-yne and its isomerization product
2-ethynyl-1,3-butadiene were observed at reaction temperatures
that are probably too low for dissociation of 1,5-hexadiyne back
to two propargyl radicals. On the current potential energy
surfaces the only route to 12HD5Y from 15HD is via dissocia-
tion and recombination, and the most recent work indicates that
the PES may need to be modified to include a direct route
between 15HD and 12HD5Y. Last, a high-temperature fulvene
to benzene route, predicted by the PES, is confirmed by our
experimental evidence.
Mechanism of Formation of 2-Ethynyl-1,3-butadiene.
2-ethynyl-1,3-butadiene appears between 1150 and 1300 K with
a maximum mole fraction of 0.02 in these experiments. This
species can only be formed from 1,2-hexadiene-5-yne, a species
that is inaccessible on the Miller and Klippenstein PES when
starting with 1,5-hexadiyne without first dissociating 15HD to
propargyl radicals. In the low-concentration kinetic work, 1,2-
hexadiene-5-yne was observed but the concentrations were too
low to measure quantitatively. In the higher concentration
samples prepared for GC-mi-FTIR-MS analysis a small but
well formed peak was observed whose spectrum confirmed that
the species was 1,2-hexadiene-5-yne, and comparison between
the FTIR analyses and the GC-MS, GC-FID analyses indicates
that trace amounts of 1,2-hexadiene-5-yne are present in the
kinetic samples. A second potential route to 2-ethynyl-1,3-
butadiene not involving dissociation of 15HD is from the
isomerization of benzene through fulvene, and this has been
observed by Nakashima et al.37 in very vibrationally hot
benzene. However, in the present thermally excited work it is
very unlikely that the temperatures are high enough to drive
benzene back to 2-ethynyl-1,3-butadiene. The presence of trace
amounts of 1,2-hexadiene-5-yne tend to suggest that some of
the original 1,5-hexadiyne has either decomposed to propargyl
radicals that have then recombined with a fraction forming
12HD5Y or that there is a direct isomerization path from 15HD
to 12HD5Y that is not included on the Miller and Klippenstein
PES.
Acknowledgment. We thank Dr L. B. Harding of Argonne
National Laboratories for performing the DFT calculations that
were used in interpreting the FTIR spectra. R.S.T., W.T., and
K.B. are grateful to the National Science Foundation for support
under contract CTS 0109053. K.B.A. gratefully acknowledges
the support of the Office of Basic Energy Sciences, Division
of Chemical Sciences, Geosciences, and Biosciences, under
contract number W-31-109-ENG-38.
Some preliminary simulations have been performed to try to
assess the relative importance of dissociation of 15HD to two
propargyl radicals, reverse of reaction 2, and isomerization of
15HD to 12HD5Y. A rate coefficient for dissociation of 15HD
to two propargyls, k-2 (reaction 2), was obtained from a QRRK
calculation by Dean.38 Rates for reactions 2 and 3 were taken
from ref 18. There does not appear to be a published rate
coefficient expression for reaction 4, and this was estimated to
be half of that for reaction 2 on the basis of Alkemade and
Homann’s product distributions. For the isomerization of 15HD
to 12HD5Y we have used the rate coefficient expression for a
1,3 H-atom shift in propyne to give allene.39 The results of this
preliminary and necessarily crude modeling indicate that at
temperatures above 1100 K dissociation of 15HD to propargyl
can be significant but that recombination to 15HD, reaction 2,
is the favored fate of the propargyl radicals with small amounts
forming 1245HT and 12HD5Y in approximately 1.5:2 propor-
tions, which is roughly similar to the distribution seen by
Alkemade and Homann. The model also indicates that direct
isomerization of 15HD to 12HD5Y is negligible. However, these
results should be treated with caution. If, as the model predicts,
1245HT and 12HD5Y are formed in 1.5:2 ratio then 1245HT
should have been observed in the analysis of the postshock
samples and there is absolutely no indication that this species
is present even in the concentrated samples prepared for GC-
mi-FTIR-MS analysis. It is therefore suggested that the
isomerization of 15HD to 12HD5Y may be more significant
than indicated by this preliminary modeling work and a thorough
theoretical investigation of the mechanism may be warranted.
Supporting Information Available: Tables of experimental
data containing reaction conditions and species concentrations.
This material is available free of charge via the Internet at http://
pubs.acs.org.
References and Notes
(1) Miller, J. A. Proc. Combust. Inst. 1996, 20, 461.
(2) Miller, J. A. Faraday Discuss. 2001, 119, 461.
(3) Richter, H.; Howard, J. B. Prog. Energy Combust. Sci. 2000, 26,
565.
(4) D’Anna, A.; Violi, A.; D’Allessio, A. Combust. Flame 2000, 121,
418.
(5) Kern, R. D.; Chen, H.; Kiefer, J. H.; Mudipalli, P. S. Combust.
Flame 1995, 100, 177.
(6) Lindstedt, P. Proc. Combust. Inst. 1998, 27, 269.
(7) Alkemade, U.; Homann, K. H. Z. Phys. Chem. 1989, 161, 19.
(8) Fahr, A.; Nayak, A. Int. J. Chem. Kinet. 2000, 32, 118.
(9) Shafir, E. V.; Slagle, I. R.; Knyazev, V. D. J. Phys. Chem. A 2003,
107, 8893.
(10) Scherer, S.; Just, T.; Frank, P. Proc. Combust. Inst. 2000, 28, 1511.
(11) DeSain, J. D.; Taatjes, C. A. J. Phys. Chem. A 2003, 107, 4843.
(12) Thomas S. D.; Communal F.; Westmoreland, P. R. ACS, DiV. Fuel
Chem., 1991, 1449.
(13) Miller, J. A.; Melius, C. F. Combust. Flame 1992, 91, 21.
(14) Melius, C. F.; Miller, J. A.; Evleth, E. M. Proc. Combust. Inst.
1992, 24, 621.
(15) Miller, J. A.; Klippenstein, S. J. J. Phys. Chem. A 2001, 105, 7254.
(16) Klippenstein, S. J.; Miller, J. A. J. Phys. Chem. A 2002, 106, 9267.
(17) Carstensen, H.-H., Dean, A. M. Proceedings of the Third Joint
Meeting of the U.S. Sections of The Combustion Institute, Chicago, March,
16-18, 2003.
(18) Carstensen, H.-H.; Dean, A. M. Private communication.
(19) Miller, J. A.; Klippenstein, S. J. J. Phys. Chem. A 2003, 107, 7783.
(20) Huntsman, W. D.; Wristers, H. J.J. Am. Chem. Soc. 1967, 18, 342.
(21) Huntsman, W. D. Intra-Sci. Chem. Rep. 1972, 6, 151.
(22) Coller, B. A. W.; Heffernan, M. L.; Jones, A. J. Aust. J. Chem.
1968, 21, 1807.
Conclusions
An extensive experimental study of the pyrolysis of 1,5-
hexadiyne has been performed at four reaction pressures of 25,
50, 300, and 500 bar and temperatures from 780 to 1400 K.
(23) Kent, J. E., Jones, A. J. Aust. J. Chem. 1970, 23, 1059.
(24) Henry, T. J.; Bergman, H. G. J. Am. Chem. Soc. 1972, 9, 5103.