Ab initioCCSD(T)cc-pVTZ//B3LYP6-311G** and CCSD(T)/complete basis set (CBS) calculations of stationary points on the C6H3 potential energy surface have been performed to investigate the reaction mechanism of C2H with diacetylene and C4H with acetylene. Totally, 25 different C6H3 isomers and 40 transition states are located and all possible bimolecular decomposition products are also characterized. 1,2,3- and 1,2,4-tridehydrobenzene and H2CCCCCCH isomers are found to be the most stable thermodynamically residing 77.2, 75.1, and 75.7kcalmol lower in energy than C2H+C4H2, respectively, at the CCSD(T)/CBS level of theory. The results show that the most favorable C2H+C4H2 entrance channel is C2H addition to a terminal carbon of C4H2 producing HCCCHCCCH, 70.2kcalmol below the reactants. This adduct loses a hydrogen atom from the nonterminal position to give the HCCCCCCH (triacetylene) product exothermic by 29.7kcalmol via an exit barrier of 5.3kcalmol. Based on Rice–Ramsperger–Kassel–Marcus calculations under single-collision conditions, triacetylene+H are concluded to be the only reaction products, with more than 98% of them formed directly from HCCCHCCCH. The C2H+C4H2 reaction rate constants calculated by employing canonical variational transition state theory are found to be similar to those for the related C2H+C2H2 reaction in the order of magnitude of 1010cm3molecule1s1 for T=29863K, and to show a negative temperature dependence at low T. A general mechanism for the growth of polyyne chains involving C2H+H(CC)nHH(CC)n+1H+H reactions has been suggested based on a comparison of the reactions of ethynyl radical with acetylene and diacetylene. The C4H+C2H2 reaction is also predicted to readily produce triacetylene+H via barrierless C4H addition to acetylene, followed by H elimination.

1.
N.
Sarker
,
A.
Somogyi
,
J. I.
Lunine
, and
M. A.
Smith
,
Astrobiology
3
,
719
(
2003
).
E.
Wilson
,
Chem. Eng. News
83
,
6
(
2005
).
3.
Y. L.
Yung
,
M.
Allen
, and
J. P.
Pinto
,
Astrophys. J., Suppl. Ser.
55
,
465
(
1984
).
4.
B.
Letourneur
and
A.
Coustenis
,
Planet. Space Sci.
41
,
593
(
1993
);
T.
Hidayat
,
A.
Marten
,
B.
Bezard
,
D.
Gautier
,
T.
Owen
,
H. E.
Matthews
, and
G.
Paubert
,
Icarus
133
,
109
(
1998
).
5.
R. A.
Marcus
,
J. Chem. Phys.
121
,
8201
(
2004
).
6.
D. W.
Clarke
and
J. P.
Ferris
,
Icarus
127
,
158
(
1997
);
[PubMed]
T.
Hidayat
,
A.
Marten
,
B.
Bezard
,
T.
Owen
,
H. E.
Matthews
, and
G.
Paubert
,
Icarus
126
,
170
(
1997
).
7.
J. I.
Lunine
,
Y. L.
Yung
, and
R. D.
Lorenz
,
Planet. Space Sci.
47
,
1291
(
1999
).
8.
M. A.
Gurwell
,
Astrophys. J. Lett.
616
,
L7
(
2004
).
9.
A. S.
Wong
,
C. G.
Morgan
,
Y. L.
Yung
, and
T.
Owen
,
Icarus
155
,
382
(
2002
).
10.
J. H.
Waite
, Jr.
,
H.
Niemann
,
R. V.
Yelle
,
W. T.
Kasprzak
,
T. E.
Cravens
,
J. G.
Luhmann
,
R. L.
McNutt
,
W.-H.
Ip
,
D.
Gell
,
V.
De La Haye
,
I.
Mueller-Wordag
,
B.
Magee
,
N.
Borggren
,
S.
Ledvina
,
G.
Fletcher
,
E.
Walter
,
R.
Miller
,
S.
Scherer
,
R.
Thorpe
,
J.
Xu
,
B.
Block
, and
K.
Arnett
,
Science
308
,
982
(
2005
).
11.
Y. L.
Yung
and
W. D.
De More
,
Photochemistry of Planetary Atmospheres
(
Oxford University Press
,
Oxford
,
1999
).
12.
A.-S.
Wong
,
Y. L.
Yung
, and
A. J.
Friedson
,
Geophys. Res. Lett.
30
,
1447
, DOI:10.1029/2002GL016661 (
2003
).
13.
E. H.
Wilson
and
S. K.
Atreya
,
Planet. Space Sci.
51
,
1017
(
2003
).
14.
W. M.
Jackson
and
A.
Scodinu
,
Astrophys. Space Sci. Lib.
311
,
85
(
2004
);
G.
Apaydin
,
W. H.
Fink
, and
W. M.
Jackson
,
J. Chem. Phys.
121
,
9368
(
2004
);
[PubMed]
N. S.
Smith
and
F.
Raulin
,
J. Geophys. Res.
104
,
1873
, DOI:10.1029/1998JE900027 (
1999
).
15.
N. S.
Smith
,
Y.
Benilan
, and
P.
Bruston
,
Planet. Space Sci.
46
,
1215
(
1998
).
16.
J. H.
Wang
,
K.
Liu
,
Z.
Min
,
H.
Su
,
R.
Bersohn
,
J.
Preses
, and
J. Z.
Larese
,
J. Chem. Phys.
113
,
4146
(
2000
).
17.
R. J.
Cody
,
P. N.
Romani
,
F. L.
Nesbitt
,
M. A.
Iannone
,
D. C.
Tardy
, and
L. J.
Stief
,
J. Geophys. Res.
108
,
5119
, DOI:10.1029/2002JE002037 (
2003
);
R. J.
Cody
,
W. A.
Payne
,Jr.
,
R. P.
Thorn
,Jr.
,
F. L.
Nesbitt
,
M. A.
Iannone
,
D. C.
Tardy
, and
L. J.
Stief
,
J. Phys. Chem. A
106
,
606
(
2002
);
G. P.
Smith
,
Chem. Phys. Lett.
376
,
381
(
2003
);
M. J.
Davis
and
S. J.
Klippenstein
,
J. Phys. Chem. A
106
,
5860
(
2002
).
18.
K.
Seki
and
H.
Okabe
,
J. Phys. Chem.
97
,
5284
(
1993
);
B. A.
Balko
,
J.
Zhang
, and
Y. T.
Lee
,
J. Chem. Phys.
94
,
7958
(
1991
);
A.
Läuter
,
K. S.
Lee
,
K. H.
Jung
,
R. K.
Vatsa
,
J. P.
Mittal
, and
H.-R.
Volpp
,
Chem. Phys. Lett.
358
,
314
(
2002
);
A. M.
Wodtke
and
Y. T.
Lee
,
J. Phys. Chem.
89
,
4744
(
1985
);
J.
Segall
,
Y.
Wen
,
R.
Lavi
,
R.
Singer
, and
C.
Wittig
,
J. Phys. Chem.
95
,
8078
(
1991
);
H.
Okabe
,
J. Chem. Phys.
78
,
1312
(
1983
).
19.
S.-H.
Lee
,
Y. T.
Lee
, and
X.
Yang
,
J. Chem. Phys.
120
,
10983
(
2004
);
[PubMed]
E. F.
Cromwell
,
A.
Stolow
,
M. J. J.
Vrakking
, and
Y. T.
Lee
,
J. Chem. Phys.
97
,
4029
(
1992
);
B. A.
Balko
,
J.
Zhang
, and
Y. T.
Lee
,
J. Chem. Phys.
97
,
935
(
1992
);
A. H. H.
Chang
,
A. M.
Mebel
,
X.-M.
Yang
,
S. H.
Lin
, and
Y. T.
Lee
,
Chem. Phys. Lett.
287
,
301
(
1998
);
J. J.
Lin
,
D. W.
Hwang
,
Y. T.
Lee
, and
X.
Yang
,
J. Chem. Phys.
109
,
2979
(
1998
);
A.
Peña-Gallergo
,
E.
Martínez-Núñez
, and
S. A.
Vázquez
,
Chem. Phys. Lett.
353
,
418
(
2002
).
20.
M.
Allen
,
J. P.
Pinto
, and
Y. L.
Yung
,
Astrophys. J.
242
,
L125
(
1980
).
21.
L. M.
Lara
,
E.
Lellouch
,
J. J.
Lopez-Moreno
, and
R.
Rodrigo
,
J. Geophys. Res.
101
,
23261
, DOI:10.1029/96JE02036 (
1996
).
22.
M. C.
Gazeau
,
H.
Cottin
,
V.
Vuitton
,
N.
Smith
, and
F.
Raulin
,
Planet. Space Sci.
48
,
437
(
2000
).
23.
C. N.
Keller
,
V. G.
Anicich
, and
T. E.
Cravens
,
Planet. Space Sci.
46
,
1157
(
1998
).
24.
M.
Banaszkiewicz
,
L. M.
Lara
,
R.
Rodrigo
,
J. J.
Lopez-Moreno
, and
G. J.
Molina-Cuberos
,
Icarus
147
,
386
(
2000
);
P.
Rannou
,
F.
Hourdin
,
C. P.
McKay
, and
D.
Luz
,
Icarus
170
,
443
(
2004
).
25.
D.
Toublanc
,
J. P.
Parisot
,
J.
Brillet
,
D.
Gautier
,
F.
Raulin
, and
C. P.
McKay
,
Icarus
113
,
2
(
1995
);
[PubMed]
L. M.
Lara
,
E.
Lellouch
, and
V.
Shematovich
,
Astron. Astrophys.
341
,
312
(
1999
).
26.
E. H.
Wilson
and
S. K.
Atreya
,
J. Geophys. Res.
109
,
E06002
, DOI:10.1029/2003JE002181 (
2004
).
27.
R. D.
Lorenz
,
C. P.
McKay
, and
J. I.
Lunine
,
Science
275
,
642
(
1997
).
28.
E. H.
Wilson
,
S. K.
Atreya
, and
A.
Coustenis
,
J. Geophys. Res.
108
,
5014
, DOI:10.1029/2002JE001896 (
2003
).
29.
T. L.
Roush
and
J. B.
Dalton
,
Icarus
168
,
158
(
2004
).
30.
R.
Lorenz
and
J.
Mitton
,
Lifting Titan’s Veil
(
Cambridge University Press
,
Cambridge
,
2002
).
31.
J. O. P.
Pedersen
,
B. J.
Opansky
, and
S. R.
Leone
,
J. Phys. Chem.
97
,
6822
(
1993
).
32.
H.
Van Look
and
J.
Peeters
,
J. Phys. Chem.
99
,
16284
(
1995
).
33.
B.
Ceursters
,
H. M. T.
Nguyen
,
J.
Peeters
, and
M. T.
Nguyen
,
Chem. Phys.
262
,
243
(
2000
).
34.
D.
Chastaing
,
P. L.
James
,
I. R.
Sims
, and
I. W. M.
Smith
,
Faraday Discuss.
109
,
165
(
1998
).
35.
R. I.
Kaiser
,
F.
Stahl
,
P. v. R.
Schleyer
, and
H. F.
Schaefer
 III
,
Phys. Chem. Chem. Phys.
4
,
2950
(
2002
).
36.
T. N.
Le
,
A. M.
Mebel
, and
R. I.
Kaiser
,
J. Comput. Chem.
22
,
1522
(
2001
).
37.
R. K.
Frost
,
G. S.
Zavarin
, and
T. S.
Zwier
,
J. Phys. Chem.
99
,
9408
(
1995
).
38.
C.
Xu
,
M.
Braun-Unkhoff
,
C.
Naumann
, and
P.
Frank
,
Proc. Combust. Inst.
31
,
231
(
2007
).
39.
Y.
Guo
,
X.
Gu
,
F.
Zhang
,
A. M.
Mebel
, and
R. I.
Kaiser
,
Phys. Chem. Chem. Phys.
9
,
1972
(
2007
).
40.
H. F.
Bettinger
,
P. v. R.
Schleyer
, and
H. F.
Schaefer
 III
,
J. Am. Chem. Soc.
121
,
2829
(
1999
).
41.
H. M. T.
Nguyen
,
T.
Holtzl
,
G.
Gopakumar
,
T.
Veszpremi
,
J.
Peeters
, and
M. T.
Nguyen
,
Chem. Phys.
316
,
125
(
2005
).
42.
A. D.
Becke
,
J. Chem. Phys.
98
,
5648
(
1993
).
43.
C.
Lee
,
W.
Yang
, and
R. G.
Parr
,
Phys. Rev. B
37
,
785
(
1988
).
44.
See EPAPS Document No. E-JCPSA6-128-001822 for optimized geometries, rotational constants, vibrational frequencies, and total B3LYP6-311G** energies and ZPE of all species on the C6H3 PES. For more information on EPAPS, see http://www.aip.org/pubservs/epaps.html.
45.
G. D.
Purvis
and
R. J.
Bartlett
,
J. Chem. Phys.
76
,
1910
(
1982
);
G. E.
Scuseria
,
C. L.
Janssen
, and
H. F.
Schaefer
III
,
J. Chem. Phys.
89
,
7382
(
1988
);
G. E.
Scuseria
and
H. F.
Schaefer
III
,
J. Chem. Phys.
90
,
3700
(
1989
);
J. A.
Pople
,
M.
Head-Gordon
, and
K.
Raghavachari
,
J. Chem. Phys.
87
,
5968
(
1987
).
46.
T. H.
Dunning
, Jr.
,
J. Chem. Phys.
90
,
1007
(
1989
).
47.
K. A.
Peterson
and
T. H.
Dunning
, Jr.
,
J. Chem. Phys.
99
,
3898
(
1995
).
48.
K. M.
Ervin
,
S.
Gronert
,
S. E.
Barlow
,
M. K.
Gilles
,
A. G.
Harrison
,
V. M.
Beirbaum
,
C. H.
DePuy
,
W. C.
Lineberger
, and
G. B.
Ellison
,
J. Am. Chem. Soc.
112
,
5750
(
1990
).
49.
M. J.
Frisch
,
G. W.
Trucks
,
H. B.
Schlegel
 et al., GAUSSIAN 98, Revision A.9,
Gaussian, Inc.
, Pittsburgh, PA,
1998
.
50.
MOLPRO, a package of ab initio programs written by
H.-J.
Werner
and
P. J.
Knowles
, Version 2002.6, R. D. Amos et al.,
University of Birmingham
: Birmingham, UK,
2003
.
51.
M.
Sayes
,
M.-F.
Reyniers
,
G. B.
Marin
,
V.
Van Speybroeck
, and
M.
Waroquier
,
J. Phys. Chem. A
107
,
9147
(
2003
).
52.
D. K.
Malick
,
G. A.
Petersson
, and
J. A.
Montgomery
,
J. Chem. Phys.
108
,
5704
(
1998
).
53.
V. V.
Kislov
,
T. L.
Nguyen
,
A. M.
Mebel
,
S. H.
Lin
, and
S. C.
Smith
,
J. Chem. Phys.
120
,
7008
(
2004
).
54.
A. M.
Mebel
,
M. C.
Lin
,
D.
Chakraborty
,
J.
Park
,
S. H.
Lin
, and
Y. T.
Lee
,
J. Chem. Phys.
114
,
8421
(
2001
).
55.
L. K.
Madden
,
L. V.
Moskaleva
,
S.
Kristyan
, and
M. C.
Lin
,
J. Phys. Chem. A
101
,
6790
(
1997
).
56.
L. V.
Moskaleva
,
L. K.
Madden
, and
M. C.
Lin
,
Phys. Chem. Chem. Phys.
1
,
3967
(
1999
).
57.
J.
Troe
and
V. G.
Ushakov
,
J. Chem. Phys.
115
,
3621
(
2001
).
59.
F.
Goulay
and
S. R.
Leone
,
J. Phys. Chem. A
110
,
1875
(
2006
).
60.
Y.
Georgievskii
and
S. J.
Klippenstein
,
J. Chem. Phys.
122
,
194103
(
2005
).
61.
P. J.
Linstrom
, in
NIST Chemistry WebBook
, NIST Standard Reference Database Number 69, edited by
W. G.
Mallard
(
National Institute of Standards and Technology
, Gaithersburg,
2003
), http://webbook.nist.gov/chemistry/.
62.
J.
Cernicharo
,
A. M.
Heras
,
A. G. G. M.
Tielens
,
J. R.
Pardo
,
F.
Herpin
,
M.
Guélin
, and
L. B. F. M.
Waters
,
Astrophys. J.
546
,
L123
(
2001
).

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