Letters to the Editor
6947
are a fair model for those of the analogous ‘‘free’’ or bimo-
lecular reaction, CH4ϩO(1D2). The observed14 rovibrational
distribution, P( ,J), for nascent OH formed from the
v
CH •O clusters is almost identical to the P( ,J) of the free
v
4
3
reaction.9 This suggests that the presence of the O2 as a third
body in the complex does not radically influence the energet-
ics and that there is a similar reaction mechanism for the
cluster and free reactions. Since almost all of E† arises from
the reaction exothermicity, not the kinetic energy from ozone
photolysis, reduction of E† due to a ‘‘squeezed atom’’
effect19,20 is unimportant. Additionally, P( ϭ0,J) was mea-
v
sured using the fast photolysis laser and a high resolution
probe laser and found to be indistinguishable from that mea-
sured using a ns photolysis laser.14
From the classical chemical quenching experiments1,2
a
*
lifetime for the CH3OH intermediate of 0.8 ps was deduced.
This value was the slope-to-intercept ratio of N2/CH3OH vs
CH4 pressure following photolysis of nitrous oxide,
N2Oϩh185 nm→N2ϩO(1D2). A significant correction for
the putative unquenchable fast channel was made to the data,
and an E†-independent quenching rate constant of 2ϫ1011
MϪ1 sϪ1 ͑3ϫ10Ϫ10 cm3 sϪ1͒ was assumed to deduce the 0.8
ps value. As discussed by Tsang,2 these experiments1 did not
determine whether the O(1D2) was thermalized prior to re-
action, thereby creating an uncertainty up to 7800 cmϪ1 in
FIG. 1. Laser-induced fluorescence signal from OH( ϭ0) as a function of
v
photolysis/probe time delay for CH4•O3ϩh nm→CH3ϩOHϩO2 . For the
267
lower trace, the probe wavelength was 306.1 nm, probing mostly OH X(
v
ϭ0, high-J͒ states. For the upper trace the probe wavelength was 308.0 nm,
probing mostly low-J states.22 The smooth curves through the data are fits to
the functional form, LIF(tD)ϭ1Ϫexp(ϪtD/) for ϭ3 ps. Shown near
tDϭ0 in the upper trace is the integral of the laser cross-correlation.
nonlinear least-squares fit to many data sets yielded ϭ3 ps,
with no significant differences between the two probe wave-
lengths. Values of less than 2.2 ps or greater than 3.8 gave
fits that looked poor, and the goodness-of-fit parameter, 2,
became much larger than its minimum value. Fitting with a
sum of exponentials, LIF(tD)ϭ⌺ici͓1Ϫexp (ϪtD/i)], did
*
the energy content of the CH3OH . Because of these uncer-
tainties and the different nature of the two experiments, the
difference between 0.8 ps and the 3 ps reported here is not
surprising.
2
not decrease by more than two percent, so given the
*
In addition to OH from the long-lived CH3OH com-
present signal-to-noise ratio, the data were fit by a single
risetime. The laser pulse durations in this experiment are
much shorter than the reaction time, so deconvolution of the
pulse duration is unimportant. Also shown in Fig. 1 is the
numerical integral of the experimental cross correlation,
which would be the LIF time dependence if the transition
state were very short lived.
plex, in the free reaction a major fraction of the OH was
hypothesized to be formed via a short-lived intermediate that
is not quenched in the classical chemical studies. In the laser
studies7–13 of OH product P( ,J), this prompt channel sup-
v
posedly yields OH in high rovibrational states and accounts
for most of OH formed. OH( ϭ0) even in low rotational
v
states is from the RRKM-like reaction channel.9 While the
spectral breadth of a fast laser does not permit probing a
single rotational level, the OH rise times at 308.0 m ͑mostly
low-J͒ and 306.1 nm ͑mostly high-J͒ are the same. No evi-
dence was seen for a fast OH component. Given the time
resolution and signal-to-noise of these experiments, any
prompt OH channel must produce less than 13% of the OH
probed at 308.0 nm and less than 20% of that probed at
306.1 ns.29 It is conceivable that vibrationally excited OH
produced in rovibrational states not yet probed is formed
through a short-lived intermediate.
It seems reasonable to interpret the observed 3 ps rise-
*
time of OH as being the decay time of a CH3OH interme-
diate ͑cf. also Refs. 18–21͒. The dissociation,
O3ϩh267 nm→O(1D2)ϩO2(1⌬g) is prompt23–25 ͑DISSϽ15
fs͒ and the average kinetic energy release26,27 is ϳ4550 cmϪ1
͑O atom velocity of ϳ2.1 nm psϪ1͒, so a direct process, not
involving a long-lived intermediate, should be very fast. Fur-
thermore, the value of 3 ps is comparable to the lifetime
calculated
from
Rice–Ramsburger–Kassel–Marcus
͑RRKM͒ theory for the dissociation of methanol at the level
of excitation of these experiments. The RRKM lifetime,
calculated28 using the vibrational frequencies and rotational
constants for the CH3OH activated complex determined by
Tsang2 to reproduce the experimental thermal rate constant
parameters for the reaction CH3OH→CH3ϩOH, is ϳ2 ps for
an energy, E†, 16 500 cmϪ1 above the thermodynamic
threshold (E†ϭ⌬HϩEtransϭ14 980ϩ1515 cmϪ1͒. Agree-
ment with an RRKM calculation at a single energy is not
definitive, and until has been measured for many energies
and H/D isotopic substitution experiments are completed,
one may only claim that the present results are consistent
with statistical theory.
We thank the U.S. Air Force Office of Scientific Re-
search for support and M. P. Casassa, E. J. Heilweil, and D.
S. King for valuable discussions and suggestions. R.D.v.Z.
acknowledges receipt of an NRC/NIST. In fact, supposedly
only a minority of postdoctoral associateship. E-mail:
vanzee@micf.nist.gov or jcs@enh.nist.gov
1 C-L. Lin and W. B. DeMore, J. Phys. Chem. 77, 863 ͑1973͒.
2 W. Tsang, Int. J. Chem. Kinet. 8, 193 ͑1976͒. See works cited here for
classical chemical literature on CH4ϩO(1D2).
3 R. I. Greenberg and J. Heicklen, Int. J. Chem. Kinet. 4, 417 ͑1972͒.
4 P. Casavecchia, R. J. Buss, S. J. Sibener, and Y. T. Lee, J. Chem. Phys. 73,
6351 ͑1980͒.
One may question whether the dynamics in the cluster
J. Chem. Phys., Vol. 102, No. 17, 1 May 1995
150.135.239.97 On: Thu, 18 Dec 2014 08:00:27