HONO and HONO-Water
J. Phys. Chem. A, Vol. 101, No. 34, 1997 6013
of near-UV photons in this spectral region results in dissociation
according to eq 1 via a relatively long-lived excited state.8,24 In
the electronic ground state HONO occurs in two rotameric forms
separated by a large internal rotation barrier, a more stable and
abundant anti rotamer and an energetically disfavored syn
conformer that is less stable by 2.7 kJ mol-1. The equilibrium
constant at 277 K has been determined as
tively, cluster photodissociation makes a significant contribution
to the production of rotationlly hot NO(V′′ ) 2). These two
alternatives can be distinguished in principle by measurements
of the NO alignment. A substantial reduction in the alignment
A(2) of NO(V′′ ) 2) from the limiting value of +0.8 to +0.27
0
has been reported for the 355 nm dissociation of HONO at
ambient temperature, but this may also be attributed to overall
rotation of the parent during the lifetime of the excited
molecule.8,24
K ) Nanti /Nsyn ) 3.25
(7)
Photodissociation of HONO Clusters. The low J part of
the NO(V′′ ) 2) photofragment rotational distribution clearly
has a dynamical origin very different from the Gaussian
component. Shifts in the rotational distribution of photofrag-
ments toward much lower angular momenta have been observed
before on clustering of molecules and can be explained by
channeling excess energy and momenta into additional degrees
of freedom associated with cluster coordinates.4-6 Less energy
and smaller fractions of the phase space will be available for
partitioning energy and angular momentum into the photofrag-
ments. The photodissociation of bare HONO and its alkyl
derivatives gives rise to highly rotationally inverted NO.
Complexation on jet-cooling can therefore be identified readily
by the production of NO in low angular momentum states as
noted previously for tert-butyl nitrite.29 Kades et al. have
recently studied the production of vibrationally excited NO in
the near-UV photodissociation of CH3ONO and (CH3)3CONO
clusters30 and attributed the low J part of the observed bimodal
rotational distributions to clusters of the type [RONO]n with a
broad size distribution ranging from n ) 2 to n ) 20.30
We explain the Boltzmann-like component with Trot ) 170
K in our rotational distribution for NO(V′′ ) 2) by the
photodissociation of mixed HONO-water clusters. We have
argued that the complexes HONO-H2O and HONO(H2O)n are
likely to prevail as the precursor species but cannot of course
exclude a broad cluster size distribution, although the observed
significant retention of the vibrational excitation of NO by
by Bongartz et al.16 The presence of two distinct conformers
with slightly shifted electronic spectra gives rise to an over-
lapped, composite electronic absorption in the near-UV that is
dominated at 300 K by the anti conformer. The characteristic
vibronic features forming progressions in the NdO stretching
mode of the A˜ states of each conformer are interpreted as
transitions to quasi-bound levels supported by a shallow well
along the O-N dissociation coordinate. Alternatively, they may
be described as short-lived resonances decaying by the dis-
sociation of the weak, central O-N bond. The lifetimes of these
levels appear to increase with n*, the number of quanta in the
NdO stretching vibration of the excited state, and hence, with
transition energy as judged from the decrease in their spectral
widths.24 Excitation of these resonances can lead to vibrational
adiabatic dissociation with retention of the vibration of the NdO
fragment and to dissociation by conversion of NdO vibrational
motion on the excited-state surface into translation along the
dissociation coordinate. Excitation at 355 nm coincides with
the 220 or n* ) 2 resonance of the prevailing anti rotamer with
two quanta in the NdO stretching vibration of the excited state.
The vibrational distribution of the NO fragment from the
photolysis of 300 K HONO on this band has been measured by
Dixon and Rieley and may be compared with distributions
calculated by Henning et al.27 and Cotting and Huber.24 Both
experiment and theory indicate that the n* ) 2 resonance decays
preferentially by the nonadiabatic route with loss of one
vibrational quantum:
complexed HONO on excitation of the 22 feature at 355 nm
0
indicates that the anti-HONO chromophore is not disturbed
significantly by cluster formation. Significant hydration of
HONO will shift the absorption spectrum of HONO to the blue
in the direction of the broadened spectrum of the aqueous acid.
A blue shift on complexation with water will favor excitation
of lower quanta in the excited state at 355 nm.. Furthermore,
vibrational relaxation during expulsion of the NO fragment from
larger clusters is expected to reduce the yield of NO(V′′ ) 2),
whereas significant retention is observed. We therefore prefer
the binary complex HONO-H2O and small clusters of the type
HONO(H2O)n with n ) 2-5 as the most likely parents of the
observed rotationally cold NO(V′′ ) 2) distribution. The
vibrational state distribution of NO from the near-UV photo-
dissociation of tert-butyl nitrite, where H-bonding in the
clustered parent is unimportant, does not appear to be altered
drastically by cluster formation. In that case some broadening
of the high J Gaussian part of the rotational distribution of NO
has also been observed but has been attributed to the photo-
dissociation of the clustered parent molecules.31
HOsNdO(A˜ 1A′′ n* ) 2) f
HO(X2Π) + NdO(2Π , V′′ ) 1) (8)
Our measurements relate to excitation of the n* ) 2 resonance
of jet-cooled HONO and to the adiabatic channel leading to
NO(V′′ ) 2). No attempt was made to measure the (V′′ ) 2)/
(V′′ ) 1) vibrational ratio of the nascent NO because of
interference from NO(V′′ ) 1) from the photodissociation of
NO2.
The rotational distribution for NO(V′′ ) 2) we have deduced
(Jmax ) 25; fwhm, ∆J ) 15) is Gaussian in shape and is in
good agreement with the previous ambient temperature mea-
surement of Dixon and Rieley8 who described their distributions
as approximately Gaussian in J with a maximum around J )
25.9 and a half width of 15.2 for the V′′ ) 2 distribution. The
distributions predicted for this channel by theory on the basis
of a quasi-triatomic model are narrower and shifted to lower or
higher J depending on the excited-state potential used.24,28 The
calculated distribution for the NO(V′′ ) 1) channel in the
dissociation of the n* ) 2 resonance has a pronounced
minimum. We were unable to measure the NO(V′′ ) 1)
rotational distribution because of strong interference from the
photodissociation of NO2.20,22 Our measurements indicate,
however, that the width of the NO(V′′ ) 2) rotational distribution
does not appear to be narrowed significantly by jet-cooling the
parent with Ar. This supports the notion that the angular
momentum disposal observed in the 355 nm photodissociation
of HONO is not described perfectly by the theory. Alterna-
Conclusions
We have developed a stable source for the continuous
generation of gaseous HONO with high number density. The
source has been used successfully for a study of photodisso-
ciation of bare HONO and of small HONO-H2O clusters in a
continuous supersonic jet expansion. Excitation of a mixture
of jet-cooled anti-HONO and small HONO-water clusters on
the 220 vibronic transition at 355 nm produces NO(V′′ ) 2) with