ϩ
the oxidation of NO2Ϫ to NO2 is reasonable. For the NO2 –NO2
could yield NH N(O)᎐NOH which could yield NH NO ϩ
᎐
2 2
NOH which would give N2 ϩ 0.5N2O ϩ 1.5H2O. We have no
evidence on this point.
couple22 EЊ is 1.51 V, and the oxidation involves a large geom-
etry change from bent to linear. Swarski et al.,24 in the course of
a study of the radiation chemistry of sodium nitrate solution in
the presence of CeIV, studied the CeIV/HNO2 reaction. They
proposed the mechanism in eqns. (13)–(16). We see no reason to
The CeIV/HNO2/HN3 system
The stoichiometric results show clearly that there is a large
excess consumption of CeIV over that expected for reactions (3)
and (5). Solutions of CeIV in sulfuric acid are very stable, and
losses by oxidation of water to O2 are negligible. This was con-
firmed by a mass-spectrometric analysis. The concentration of
nitrate ions formed is greater than the initial nitrite concen-
tration, so some of the azido nitrogen must have been oxidised.
We considered the possibility of mechanisms involving the
known intermediate N3NO formed in reaction (1) or the species
Ϫ
Ϫ
CeIV ϩ NO2
[CeIVؒNO2
]
fast
(13)
(14)
[CeIVؒNO2Ϫ] → CeIII ϩ NO2 slow
2NO2
N2O4 fast
(15)
(16)
Ϫ
N2O4 ϩ H2O
HNO2 ϩ Hϩ ϩ NO3
NNN–NO or NNN–O–N᎐O that might be formed by com-
᎐
2
bination of the radicals NO2 and N3.
modify this. The rate data of Swarski et al. when interpolated
at [H2SO4 ] = 0.725 mol dmϪ3 gave k2 = 331 dm3 molϪ1 Ϫ1, in
The rate of decomposition of nitrosyl azide, reaction (2), has
s
been found by Goldstein and Czapski28 to be >106[N3NO]
reasonable agreement with our results, assuming that their
room temperature (unspecified) was somewhat below 25 ЊC.
We have considered the possibility of an outer-sphere
mechansim. Using the simpler form of the Marcus equation25
mol dmϪ3 Ϫ1, so an encounter controlled reaction with 0.125
s
mol dmϪ3 CeIV could possibly trap N3NO before it decomposed
to N2 ϩ N2O. However, the rate of formation of N3NO is very
much less than the rates of cerium() oxidation of HNO2 and
HN3 under our conditions, so it seems unlikely that this can
account for the excess consumption of oxidant. Thus mixing
equal volumes of our stock solutions of CeIV and NaNO2 ϩ
NaN3 the calculated rates of reactions (5), (3) and (1) are 276,
48 and 0.7 mol dmϪ3 sϪ1 respectively.
22
without work terms one can use (EЊ)red and the self-
exchange constants23 for red/redϩ combined with the k8
ؒ
values for total CeIV to calculate apparent ‘self exchange con-
stants’ for CeIV/CeIII in 0.725 mol dmϪ3 sulfuric acid. Such
calculations showed no sort of self-consistency, giving values/
dm3 molϪ1 sϪ1 of 105.6 (NO2Ϫ), 109.2 (N3Ϫ) and 1015.1 (NH2OH).
These can be compared with a literature value26 of 4.2 dm3
molϪ1 sϪ1 for CeIV/CeIII in 0.4 mol dmϪ3 sulfuric acid at 0 ЊC.
We conclude that these oxidations proceed by an inner sphere
mechanism.
The molecule nitryl azide, NNN–NO2, has been made29
ϩ
Ϫ
by the reaction of NO2 with N3 in organic solvents, and is
markedly more stable than N3NO. However, it decomposes to
form dinitrogen monoxide, eqn. (18), and so although it may be
The CeIV/HNO2/N2H5؉ system
NNN–NO2 → 2N2O
(18)
The observed rate of consumption of CeIV is much faster than
the rate expected for the relatively slow CeIV/hydrazine reaction
as can be seen from Fig. 2. Comparison of the half-lifetimes
shows that the rate of consumption of CeIV is very similar to
that calculated for the rate of the hydrazine/nitrous acid reac-
tion. For [N2H5ϩ]0 = 0.035, [HNO2]0 = 0.0025, [CeIV]0 = 0.0005
mol dmϪ3 successive half-lives for CeIV are 0.0318, 00282,
0.027 s which compare with calculated values for N2H5ϩ/HNO2
of 0.027, 0.028 and 0.029 s. An exact comparison is not to be
expected because the calculated rate of the hydrazine/nitrous
acid reaction was obtained from a study10 in perchloric acid,
assuming that the rate in sulfuric acid would be the same at a
given Ho value. The results show that CeIV reacts rapidly with
an intermediate in the hydrazine/nitrous acid reaction, NH N᎐
formed by radical combination it is unlikely to be responsible
for the consumption of CeIV. The isomeric species NNN–O–
N᎐O could also be formed by radical combination, and has
᎐
been postulated as an intermediate30 to account for the prod-
ucts of the oxidation of hydrazoic acid by concentrated nitric
acid. A fragmentation reaction such as (19) would produce
NNN–O–N᎐O → N ϩ 2NO
(19)
᎐
2
nitric oxide which should be readily oxidisable to NOϩ which
would hydrate to HNO2 ϩ Hϩ. The simple form of the Marcus
equation can be used to predict a bimolecular rate constant for
an outer sphere oxidation of NO by CeIV of ca. 330 dm3 molϪ1
s
Ϫ1. Such a reaction would require 6 equivalents of CeIV to
᎐
2
NOH. There is a precursor to this species, the initial nitrosation
convert both NO molecules into nitrate and could readily
account for excess consumption of oxidant.
product NH2NHNO, and the possibility that CeIV reacts with
this before it tautomerises to NH N᎐NOH cannot be excluded.
To check whether this suggestion is reasonable we assumed
that the rate constant of combination for N3/NO2 may be
approximated as the geometric mean of the known31,32 combin-
ation rate constants of N3/N3 and NO2/NO2. A steady state
treatment based on the rates of formation and removal of N3
and NO2 leads to the prediction that the rate of combination of
N3/NO2 is ca. 1/6 of the rate of N3/N3 (which is close to the
encounter limit). Thus a reasonable assumption about the rate
of combination of N3 and NO2 predicts the formation of a
sizeable amount of the combined product, which may be, of
course, a mixture of isomers. This is, therefore, a reasonable
mechanism to account for the undoubted excess consumption
of CeIV.
The final point to discuss is the relatively slow fading of the
absorbance in the later stages of the run, which is very much
slower than would be predicted from the stopped-flow kinetics.
For example, in run 9, the half-lifetime for the consumption of
nitrite is calculated to be ca. 0.02 s, and for the reaction of azide
it should be even less. However, the absorbance changes were
measured over a period of ca. 2 min, with a half-lifetime of
᎐
2
At lower concentrations of hydrazine the rate of cerium()
consumption is somewhat less. An approximate value for the
rate constant k8 based on the assumed eqn. (17) was obtained
Ϫd[CeIV]/dt = k [CeIV][NH N᎐NOH]
(17)
᎐
9
2
by setting up a series of differential equations for d[CeIV]/dt,
d[N2H5ϩ]/dt, d[HNO ]/dt and d[NH N᎐NOH]/dt and integrat-
᎐
2
2
ing by the Gear method. A series of values for k9 was tried and
the best fit, shown in the figure, gave k9 ≈ 104 dm3 molϪ1 sϪ1
.
This fit is not perfect, and it may be that additional terms
should be included in the numerical integration. The only liter-
ature report of any related process is a study by Gupta and co-
workers27 of the cerium() reaction with hyponitrous acid
H N O . Gupta suggested oxidation of HON᎐NOH to HON᎐
᎐
᎐
2
2
2
ؒ
NO followed by a further oxidation to the acid form of
Angeli’s salt, H N O (HON(O)᎐NOH) which breaks down to
᎐
2
2
3
HNO2 and HNO, which then undergoes further reaction to
form N2, HNO3 and N2O. A similar pathway in our system
J. Chem. Soc., Dalton Trans., 1999, 3311–3316
3315