Reaction of OH with Hydrogen Peroxide
J. Phys. Chem. A, Vol. 107, No. 49, 2003 10647
-
12
12
cm3
At 200 K, expression 2 gives k1 ) (2.8 ( 0.9) × 10
Acknowledgment. The authors gratefully acknowledge the
support of this research by the National Aeronautics and Space
Administration (Grant NAG5-8923, NAG5-13339, and the
Upper Atmosphere Research Program). D.C.M. acknowledges
a National Science Foundation Graduate Research Fellowship.
S.R.L. wishes to acknowledge the many profound interactions
with Professor Charles Parmenter throughout his career.
-
1
-1
molecule s , while extrapolation of the current JPL and
2
1
-12
3
IUPAC recommendation gives k1 ) (1.3 ( 0.6) × 10 cm
-
1
-1
molecule s . Clearly, extrapolation of the currently recom-
mended value of k112,21 to the lower temperatures of the
atmosphere may result in a value of k1 that is quite inaccurate.
If k1 is indeed higher than currently recommended, atmospheric
models underestimate the loss of HOX in the upper troposphere
and lower stratosphere due to reaction R1. It is also noteworthy
that expression 2 yields values of k1 around 240-250 K that
agree well with the value of k1 at these temperatures reported
References and Notes
(
1) Baldwin, R. R.; Walker, R. W. J. Chem. Soc., Faraday Trans. 1
1979, 75, 140.
(2) Keyser, L. F. J. Phys. Chem. 1980, 84, 1659.
3) Sridharan, U. C.; Reimann, B.; Kaufman, F. J. Chem. Phys. 1980,
3, 1286.
4) Wine, P. H.; Semmes, D. S.; Ravishankara, A. R. J. Chem. Phys.
1981, 75, 4390.
6
8
by Lamb et al. and Lovejoy et al.
(
It is possible that the reaction of OH with H2O2 that we
observe at low temperatures does not yield the products quoted
for reaction R1; i.e., the reaction we observe is only producing
an OH‚‚‚H2O2 complex that is not in turn dissociating to form
H2O and HO2. However, we do not believe that this is the case.
7
(
(5) Kurylo, M. J.; Murphy, J. L.; Haller, G. S.; Cornett, K. D. Int. J.
Chem. Kinet. 1982, 14, 1149.
(6) Lamb, J. J.; Molina, L. T.; Smith, C. A.; Molina, M. J. J. Phys.
The binding energy of the OH‚‚‚H2O2 complex is predicted to
Chem. 1983, 87, 4467.
be quite small, 17.1 kJ/mol,16 so that the rate coefficient for
(7) Vaghjiani, G. L.; Ravishankara, A. R.; Cohen, N. J. Phys. Chem.
989, 93, 7833.
1
formation of the OH‚‚‚H2O2 complex, if that complex could
only dissociate back to the reactants, would be quite small at
(8) Lovejoy, E. R.; Murrels, T. P.; Ravishankara, A. R.; Howard, C. J.
J. Phys. Chem. 1990, 94, 2386.
the pressures of these experiments. Using the Troe method for
(9) Turnipseed, A. A.; Vaghjiani, G. L.; Gierczak, T.; Thompson, J.
E.; Ravishankara, A. R. J. Chem. Phys. 1991, 95, 3244.
barrierless association reactions32,33 with the binding energy,
(10) Hippler, H.; Troe, J. Chem. Phys. Lett. 1992, 92, 333.
structure, and vibrational frequencies of the OH‚‚‚H2O2 complex
reported by Wang et al.,16 we estimated an upper limit for the
termolecular rate coefficients for formation of the OH‚‚‚H2O2
complex from reactants. The estimates show that, at the gas
number densities used in the experiments (see Table 1), the
bimolecular association rate coefficient would be at least 3
orders of magnitude smaller than the observed k1 between 96
and 296 K. This is evidence that the reaction of OH with H2O2
that we are observing is producing HO2 and H2O. We attempted
to experimentally verify that HO2 is formed by reaction R1 at
low temperatures by adding NO, which should react rapidly
with HO2 to form OH,34 to the gas mixture flowing through
the Laval nozzle. These attempts were not successful due to
experimental problems and were not further pursued.
(
11) Hippler, H.; Neunaber, H.; Troe, J. J. Chem. Phys. 1995, 103,
3510.
(
12) Sander, S. P.; Friedl, R. R.; Golden, D. M.; Kurylo, M. J.; Huie,
R. E.; Orkin, V. L.; Moortgat, G. K.; Ravishankara, A. R.; Kolb, C. E.;
Molina, M. J.; Finlayson-Pitts, B. J. Chemical Kinetics and Photochemical
Data for Use in Atmospheric Studies, EValuation 14; JPL Publication No.
2-25; Jet Propulsion Laboratory: Pasadena, CA, 2003.
(
0
13) Troe, J. J. Chem. Soc., Faraday Trans. 1994, 90, 2303.
14) Brown, S. S.; Burkholder, J. B.; Talukdar, R. K.; Ravishankara,
(
A. R. J. Phys. Chem. A 2001, 105, 1605.
(15) Smith, I. W. M.; Ravishankara, A. R. J. Phys. Chem. A 2002, 106,
4
798.
(16) Wang, B.; Hou, H.; Gu, Y. Chem. Phys. Lett. 1999, 309, 274.
17) Lee, S.; Hoobler, R. J.; Leone, S. R. ReV. Sci. Instrum. 2000, 71,
(
1816.
(18) Vakhtin, A. B.; Lee, S.; Heard, D. E.; Smith, I. W. M.; Leone, S.
R. J. Phys. Chem. A 2001, 105, 7889.
(
19) Vakhtin, A. B.; Murphy, J. E.; Leone, S. R. J. Phys. Chem. A, in
press.
(20) Smith, I. W. M. J. Chem. Soc., Faraday Trans. 1997, 93, 3741.
21) Atkinson, R.; Baulch, D. L.; Cox, R. A.; Hampson, R. F.; Kerr, J.
A.; Rossi, M. J.; Troe, J. J. Phys. Chem. Ref. Data 1997, 26, 521.
22) McCabe, D. C.; Brown, S. S.; Gilles, M. K.; Talukdar, R. K.; Smith,
I. W. M.; Ravishankara, A. R. J. Phys. Chem. A 2003, 107, 7762.
23) Scatchard, G.; Kavanagh, G. M.; Ticknor, L. B. J. Am. Chem. Soc.
952, 74, 3715.
24) Kliner, D. A. V.; Farrow, R. L. J. Chem. Phys. 1999, 110, 412.
(25) Sims, I. R.; Smith, I. W. M.; Bocherel, P.; Defrance, A.; Travers,
D.; Rowe, B. R. J. Chem. Soc., Faraday Trans. 1994, 90, 1473.
26) Orkin, V. L.; Huie, R. E.; Kurylo, M. J. J. Phys. Chem. 1996, 100,
907.
Since the supersonic expansion is greatly supersaturated with
H2O2, formation of dimers and larger clusters of H2O2 could
occur within the expansion. Also, H2O2 might form clusters with
water introduced into the flow, along with H2O2, when nitrogen
is bubbled through the H2O2/H2O solution. The rate coefficients
for the reactions of OH with the H2O2 dimers and clusters could
be significantly different than k1. However, formation of dimers
and clusters should be slow at the pressures of these experiments.
(
(
(
1
(
We again used the Troe method3
2,33
and the binding energy,
(
structure, and vibrational frequencies of the Ci dimer of H2O2
8
3
5
and the H2O2-H2O complex described by Gonz a´ lez et al. to
estimate upper limits for the rate coefficients for formation of
those complexes. The estimates show that these two processes
convert no more than 0.02% of H2O2 within the available time
at the temperatures of this study; therefore they cannot affect
the observed rate of OH decay.
(
27) Taylor, B. N.; Kuyatt, C. E. Guidelines for EValuating and
Expressing the Uncertainty of NIST Measurement Results; NIST Technical
Note 1297; US Government Printing Office: Washington, DC, 1994.
(
28) Kneba, M.; Wolfrum, J. Annu. ReV. Phys. Chem. 1980, 31, 47.
(29) Smith, I. W. M.; Williams, M. D. J. Chem. Soc., Faraday Trans.
2 1985, 81, 1849.
30) Raiche, G. A.; Jeffries, J. B.; Rensberger, K. J.; Crosley, D. R. J.
Chem. Phys. 1990, 92, 7258.
31) Silvente, E.; Richter, R. C.; Hynes, A. J. J. Chem. Soc., Faraday
(
In addition to direct studies of k1 in the temperature range
needed for atmospheric purposes, further elucidation of the
mechanism of this reaction could be provided by an investigation
of the primary and secondary H/D kinetic isotope effects on k1
at low and high temperatures. Direct study of the products of
reaction R1 at temperatures below 240 K would also be helpful.
(
Trans. 1997, 93, 2821.
(32) Troe, J. J. Chem. Phys. 1977, 66, 4745.
(
33) Troe, J. J. Chem. Phys. 1977, 66, 4758.
(34) Seeley, J. V.; Meads, R. F.; Elrod, M. J.; Molina, M. J. J. Phys.
Chem. 1996, 100, 4026.
(35) Gonzalez, L.; Mo, O.; Yanez, M. J. Comput. Chem. 1997, 18, 1124.