J. Chem. Phys., Vol. 113, No. 21, 1 December 2000
Reaction of carbon with C4H6 . I
9635
deep compared to atomic carbon and the olefine. The fate of
the triplet allene complexes is governed by H loss channels
to ͑substituted͒ propargyl radicals via tight exit transition
states located about 10–25 kJmolϪ1 above the products.
Most of the initial angular momentum channels into rota-
tional excitation of the products predominantly excited to
C-like rotations. The presence of an exit barrier is docu-
mented in the center-of-mass translation energy distributions
as well as all P(ET)’s peak around 20–50 kJmolϪ1. The
exothermicities to the C3H2R (RϩCH3 or C2H3) are very
similar and range between 200 and 220 kJmolϪ1. This dem-
onstrates that the substitution of a hydrogen atom in ethylene
by a side group has little effect on the energetics of the
reaction.
Besides these similarities, there is one striking difference
in the reaction of atomic carbon with propylene and 1,3 buta-
diene. Here, the CH3 group is conserved in the reaction and
acts as a spectator. Although no H atom loss occurs from the
C2H3 group, the increased stabilization of p14 versus p15
demonstrates an enhanced delocalization of the unpaired
electron. In addition, if the cis 1,3-butadiene reacts, the side
group can be actively involved in the chemistry, since atomic
carbon can add to both terminal carbon atoms. Therefore, we
cannot regard C2H3 as a spectator side group in this case.
cal details leading to large organic molecules are only dimly
understood and possibly initiated by a recombination of two
pentadienyl radicals, cf. Sec. I. Our proposed mechanism
suggests the growth by addition of carbon atoms to unsatur-
ated molecules such as 1,3-butadiene and is supported by
recent investigations. Although our crossed beam experi-
ments did not give any proof of a cyclic C5H5 isomer, the
situation in circumstellar envelopes close to the central car-
bon star is different from the single collision conditions.
Compared to our experiments, the molecular number density
is higher, and the C5H5 chain can isomerize upon a succes-
sive collision to cyclic C5H5 isomers. In strong analogy to
combustion processes, a collision-induced trans-cis isomer-
ization of 1,3-butadiene can precede the reaction with atomic
carbon, and the pentadienyl radical can be formed via i2 and
i6.
VIII. CONCLUSIONS
The reaction between ground state carbon atoms, C͑3Pj),
and 1,3-butadiene, H2CCHCHCH2 , was studied at averaged
collision energies of 19.3, 28.0, and 38.8 kJmolϪ1 using the
crossed molecular beam technique. The carbon atom attacks
the -orbital of the butadiene molecule without a barrier via
a loose, reactantlike transition state located at the centrifugal
barrier to form a cyclopropylidene derivative. The triplet
radical rotates in a plane which is almost perpendicular to the
total angular momentum vector J around its C-axis undergo-
ing ring opening to a vinyl substituted triplet allene mol-
ecule. This complex fragments via two micro-channels
through H atom emission to form 1- and 3-vinylpropargyl
radicals, HCCCH–C H (X2A ), and H CCC–C H (X2A ),
VI. COMBUSTION CHEMISTRY APPLICATIONS
Our crossed beam studies showed explicitly that the title
reaction leads to 1- and 3-vinylpropargyl radicals,
HCCCH–C H (X2A ), and H CCC–C H (X2A ). This re-
Љ
Љ
2
3
2
2
3
action proceeds via an initial addition of C͑3Pj) to trans-1,3-
butadiene to form a three-membered ring intermediate i1 fol-
lowed by ring opening to a substituted triplet allene species
i5 and H atom emission to the products. Although these ex-
periments did not show any evidence of the cyclopentadienyl
radical which is thought to be a potential precursor to PAH
molecules, the explicit identification of chain C5H5 radicals
holds far-reaching consequences for combustion processes.
Here, Burcat and Dvinyaninov investigated the decomposi-
tion pattern of the cyclopentadienyl radical and found
HCCCHC2H3 as the main decomposition product.35 Based
on this finding it can be strongly assumed that in combustion
flames HCCCHC2H3 can undergo ring closure followed by
H atom migration to form the cyclopentadienyl radical once
the entrance barrier can be passed via a third body reaction.
Likewise, in denser reaction environments such as flames, a
collision induced trans-cis isomerization of 1,3-butadiene
prior to a C͑3Pj) addition can form the cyclopentadienyl radi-
cal via i2 and i6.
Љ
Љ
2
3
2
2
3
through tight exit transition states. The unambiguous identi-
fication of two chain isomers of C5H5 under a single colli-
sion represents a further example of a carbon-hydrogen ex-
change in reactions of ground state carbon atoms with
unsaturated hydrocarbons. In denser media such as combus-
tion flames and close to the central star of circumstellar en-
velopes, the linear isomer can show a ring closure to form
cyclic C5H5 isomers such as the cyclopentadienyl radical—a
postulated intermediate in the formation of PAHs—via
HCCCHC2H3 . Finally, a collision-induced trans-cis isomer-
ization of 1,3-butadiene prior to a C͑3Pj) addition can form
the pentadienyl radical via cyclic reaction intermediates. The
role of cyclic C5H5 isomers in these environments will be
investigated in future RRKM calculations.
ACKNOWLEDGMENTS
R.I.K. is indebted the Deutsche Forschungsgemeinschaft
for a Habilitation fellowship ͑IIC1-Ka1081/3-1͒. This work
was supported by Academia Sinica, Taiwan, the National
Science Council of R.O.C., and by the Petroleum Research
Fund of R.O.C. We are thankful to Dr. A. H. H. Chang for
her assistance with RRKM calculations. This work was per-
formed within the international astrophysics network.
VII. ASTROPHYSICAL IMPLICATIONS
Besides its potential importance in combustion chemis-
try, investigating the formation of C5H5 isomers is expected
to contribute to the modeling of formation of complex mol-
ecules in the interstellar space. Here, the PAH synthesis in
circumstellar envelopes is of crucial importance since these
molecules are considered as the condensation nuclei to form
larger carbon-rich grain materials which are considered to be
formed in carbon-rich circumstellar shells. Here, the chemi-
1 US Clean Air Act Amendment 1990.
2 R. I. Kaiser and K. Roessler, Astrophys. J. 475, 144 ͑1997͒, and references
therein.
3 N. M. Marinov et al., Combust. Flame 114, 192 ͑1998͒; N. M. Marinov
131.111.185.72 On: Thu, 11 Dec 2014 10:39:30