The HOCO radical has been successfully detected by a photoionization mass spectrometry in gas phase. The HOCO radical produced by the reaction of Cl+HCOOH (with small excess energy; 13.0 kcal mol−1) was found to be stable and its lifetime was confirmed to be very long (≳10 ms) at room temperature. On the other hand, the HOCO radical formed by the 193 nm photolysis of C2H3COOH (with large excess energy; 55.8 kcal mol−1) exhibited fast, nonexponential, and total pressure‐dependent decay. This behavior was well interpreted by a competition of dissociation and relaxation of ‘‘hot’’ radicals. Further, the decay of ‘‘hot’’ radicals showed an apparent isotope effect (DOCO/HOCO). This fact together with an energetic consideration suggests that the observed decay is dominated by a tunneling dissociation to H+CO2, which implies the importance of the tunneling in the OH+CO reaction. The vibrational relaxation rate of the HOCO radical was roughly evaluated from the pressure dependence of the decay profile of ‘‘hot’’ HOCO radicals. The rate of reaction of HOCO radical with molecular oxygen has also been determined, and appeared pressure‐independent.

1.
J. Warnatz, Combustion Chemistry, edited by W. C. Gardiner (Springer, New York, 1984), Chap. 5.
2.
J. Heicklen, Atmospheric Chemistry (Academic, New York, 1976).
3.
R.
Atkinson
,
D. L.
Baulch
,
R. A.
Cox
,
R. F.
Hampson
, Jr.
,
J. A.
Kerr
, and
J.
Troe
,
J. Phys. Chem. Ref. Data
18
,
881
(
1989
).
4.
M.
Aoyagi
and
S.
Kato
,
J. Chem. Phys.
88
,
6409
(
1988
).
5.
M.
Mozurkewich
and
S. W.
Benson
,
J. Phys. Chem.
88
,
6429
(
1984
), and references therein.
6.
K.
Kleinermanns
,
E.
Linnebach
, and
J.
Wolfrum
,
J. Phys. Chem.
89
,
2525
(
1985
);
(b)
G.
Radhakrishnan
,
S.
Bulow
, and
C.
Wittig
,
J. Chem. Phys.
84
,
727
(
1986
);
(c)
N. F.
Schren
,
L. R.
Khundkar
,
R. B.
Bernstein
, and
A. H.
Zewail
,
J. Chem. Phys.
87
,
1451
(
1987
).,
J. Chem. Phys.
7.
(a)
D. E.
Milligan
and
M. E.
Jacox
,
J. Chem. Phys.
54
,
927
(
1971
);
(b)
M. E.
Jacox
,
J. Chem. Phys.
88
,
4598
(
1988
).,
J. Chem. Phys.
8.
B.
Ruscic
,
M.
Schwartz
, and
J.
Berkowitz
,
J. Chem. Phys.
91
,
6780
(
1989
).
9.
H. E.
Radford
,
W.
Wei
, and
T. J.
Sears
,
J. Phys. Chem.
97
,
3989
(
1992
).
10.
(a)
T. J.
Sears
,
W. M.
Fawzy
, and
P. M.
Johnson
,
J. Phys. Chem.
97
,
3996
(
1992
);
(b)
J. T.
Petty
and
C. B.
Moore
,
J. Chem. Phys.
99
,
47
(
1993
).
11.
(a)
A.
Miyoshi
,
H.
Matsui
, and
N.
Washida
,
Chem. Phys. Lett.
160
,
291
(
1989
);
(b)
A.
Miyoshi
,
H.
Matsui
, and
N.
Washida
,
J. Phys. Chem.
94
,
3016
(
1990
).
12.
Reaction enthalpy was calculated using heats of formation which were quoted from Ref. 3 or estimated by the group additivity rule [S. W. Benson, Thermochemical Kinetics, 2nd ed. (Wiley-Interscience, New York, 1976)], except for HOCO (Ref. 8) and HCO2 (Ref. 14).
13.
B.
Ruscic
,
M.
Schwarz
, and
J.
Berkowitz
,
J. Chem. Phys.
91
,
6772
(
1989
).
14.
G. C.
Schatz
,
M. S.
Fitzcharles
, and
L. B.
Harding
,
Faraday Discuss. Chem. Soc.
84
,
359
(
1987
).
15.
G.
Paraskevopoulos
and
R. S.
Irwin
,
J. Chem. Phys.
80
,
259
(
1984
).
16.
The RRKM calculation was based on the energetics and structures of related species calculated by Aoyagi and Kato (Ref.4).
17.
Tunneling probability was evaluated by the WKB approximation using a one-dimensional potential energy curve given in Ref. 4.
18.
W. C. Gardiner, Jr. and J. Troe, Combustion Chemistry, edited by W. C. Gardiner (Springer, New York, 1984), Chap. 4.
19.
J. D. Lambert, Vibrational and Rotational Relaxation in Gases (Oxford University, Oxford, 1977).
20.
Based on the experimental ΔHf0 of HOCO (Ref. 8).
21.
Ab initio calculations (Refs. 4,14) showed that the dissociation threshold to H+CO2 is slightly higher than the energy of OH+CO.
22.
G.
Paraskevopoulos
and
R. S.
Irwin
,
Chem. Phys. Lett.
93
,
138
(
1982
).
23.
A. A.
Westenberg
and
W. E.
Wilson
,
J. Chem. Phys.
45
,
338
(
1966
).
24.
H.-H.
Grotheer
,
G.
Riekert
,
D.
Walter
, and
Th.
Just
,
J. Phys. Chem.
92
,
4028
(
1988
).
25.
F. L.
Nesbitt
,
W. A.
Payne
, and
L. J.
Stief
,
J. Phys. Chem.
92
,
4030
(
1988
).
This content is only available via PDF.
You do not currently have access to this content.