Mariela Videlaab, Silvia E. Braslavsky*a and José A. Olabe*b
aMax-Planck-Institut für Bioanorganische Chemie (formerly Strahlenchemie), Postfach 101365, D-45413, Mülheim an der Ruhr, Germany. E-mail: braslavskys@mpi-muelheim.mpg.de; Fax: +49 208 306 3951
bINQUIMAE and Departamento de Química Inorgánica, Analítica y Química Física, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Pab. II, Ciudad Universitaria, Buenos Aires, Argentina C1428EHA
First published on 13th October 2004
The photodetachment of NO from [MII(CN)5NO]2− with M = Fe, Ru, and Os, upon laser excitation at various wavelengths (355, 420, and 480 nm) was followed by various techniques. The three complexes showed a wavelength-dependent quantum yield of NO production Φ(NO), as measured with an NO-sensitive electrode, the highest values corresponding to the larger photon energies. For the same excitation wavelength the decrease of Φ(NO) at 20 °C in the order Fe > Ru ≫ Os, is explained by the increasing M–N bond strength and inertness of the heavier metals. Transient absorption data at 420 nm indicate the formation of the [MIII(CN)5H2O]2− species in less than ca. 1 μs for M = Fe and Ru. The enthalpy content of [FeIII(CN)5H2O]2− with respect to the parent [FeII(CN)5NO]2− state is (190 ± 20) kJ mol−1, as measured by laser-induced optoacoustic spectroscopy (LIOAS) upon excitation at 480 nm. The production of [FeIII(CN)5H2O]2− is concomitant with an expansion of (8 ± 3) ml mol−1 consistent with an expansion of the water bound through hydrogen bonds to the CN ligands plus the difference between NO release into the bulk and water entrance into the first coordination sphere. The activated process, as indicated by the relatively strong temperature dependence of the Φ(NO) values and by the temperature dependence of the appearance of the [FeIII(CN)5H2O]2− species, as determined by LIOAS, is attributed to NO detachment in less than ca. 100 ns from the isonitrosyl (ON) ligand (MS1 state).
Reports with metallonitrosyls containing classical co-ligands X have been published for the series [MIIX5–NO]n, where M is Fe, Ru, or Os and X is NH3 and amines, CN−, polypyridines, or mixed type X4L.10–12 In these complexes, NO may be formally considered a three electron donor (i.e., NO+), with strong back donation from the low-spin d6 MII centre to the π*(NO) orbital. This is an arbitrary formalism, because the valence orbitals of the [MNO] moiety are in fact highly delocalised.13 Chemical reactions of coordinated NO+ with bases (with potential release of nitrite or nitrosothiols) and light-induced M–NO electron transfer are the most important paths of NO delivery from these complexes. Emerging results with compounds of the above mentioned series provide information on the nature of the metal and coligands, as well as medium conditions that would favour or impair the trapping14 or the photodetachment of NO.15–18
In this work we focus on the pentacyanonitrosyl complexes of Fe, Ru, and Os.11 Work with the iron derivative has been a classic in photochemical studies on coordination compounds19–22 but key questions still remain as to the detailed mechanism of the processes following photoexcitation up to the NO-release. The Ru and Os analogues of sodium nitroprusside {[Fe(CN)5NO]2−, NP} have been prepared and further studied during the last two decades.23,24 We present here a study of their photoreactivity, in comparison with that of NP, with the aim of better understanding the factors controlling NO release in these complexes, given the scarce amount of systematic studies with analogue compounds comprising the elements pertaining to the three transition series.
On the basis of the generally accepted conclusion that a photoredox process operates upon primary excitation (i.e., formally an FeII–NO+ → FeIII–NO photoconversion), and that NO is subsequently released, we analyse the conditions influencing both processes. The studies with the three metal centres comprise measurements of quantum yields at different wavelengths and temperatures, and for NP in the presence of an electron acceptor macrocyclic ligand. Transient absorption after laser pulse excitation and laser-induced optoacoustic techniques are also used, in an effort to disclose the detailed mechanistic issues associated with the NO release. Comparisons are made with previous work with NP and other relevant metallonitrosyls.
The azamacrocycles 24[ane]-N8H8·8HCl and 32[ane]-N8H8·8HCl25 were provided by Professor Fernando Pina (Universidade Nova de Lisboa, Portugal).
Buffer solutions were at pH 6.5 (NaH2PO4-Na2HPO4) and pH 4.5 (acetic acid-NaOH). For the concentrations see Methods. Water was always distilled and deionized. NaNO2, NaI, and all other common reagents were used as provided without further purification.
Fluorescence quantum yields were determined with a corrected spectrofluorimeter (Spex-Fluorolog) using tryptophan in water as reference, Φf = 0.14 at 25 °C.26 The absorbances of the sample solutions in buffer at 308 nm were A308 = 0.11, 0.12, and 0.16 for M = Os, Ru, and Fe, respectively. Excitation was at 308 nm in order to obtain a full emission spectrum. For the evaluation of the Φf values, the areas under the emission curves of the corrected spectra for the sample solutions between 360 and 600 nm were compared to those of the tryptophan solution. A correction was made for the absorbance differences. No effect on the emission yield or position of the maximum was observed upon changing excitation wavelength or upon addition of NaCl (ca. 0.1 M). An approximation had to be made for the tryptophan emission under 380 nm, because no correction was available for the spectrofluorimeter for λ < 380 nm. Thus, the yields reported are more accurate in their relative than in their absolute values.
All spectral and photochemical experiments were performed with solutions of the complexes at pH 6.5 (0.1 M buffer), after Ar bubbling and kept protected from room light before irradiation.
Nitrogen monoxide quantum yield [Φ(NO)] measurements were carried out with a commercial NO detector (inNO, Nitric Oxide Measuring System, Harvard Apparatus GmbH). The system consists of an 850 mV potentiostat and a combined electrode (700 μm diameter, amiNO Series of nitrogen monoxide sensors), covered with a series of permeable membranes allowing only NO to diffuse through and react at the electrode surface, where it is oxidized. The exchange of electrons results in an electrical current directly proportional to the amount of NO diffused through the membrane, in turn proportional to the NO concentration in the solution. Calibration of the electrode in the range approximately (10–200) × 10−9M was performed by generating NO according to reaction (1), under Ar atmosphere.
H2SO4 + NaNO2 + NaI → NO + ½ I2 + H2O + Na2SO4 | (1) |
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Fig. 1 Signals and plot for calibration of the 700 μm-amiNO electrode. (a) Developed current vs. time, after zeroing the equipment; (b) linear response of the electrode (sensitivity in this case: 137 pA nM−1). |
The slopes [b/(pA J−1)] of the linear regression of the developed current (Δi) vs. absorbed energy (ΔEabs, varied by accumulating several pulses at wavelength λ of low fluence each, Fig. 2), together with the calibration slope [Cal/(pA M−1)], and the volume of solution irradiated, Vsol, were used to calculate the NO quantum yields according to eqn. (2), with E(λ) the molar energy of the laser beam at the excitation wavelength.
![]() | (2) |
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Fig. 2 Chronoamperograms of [M(CN)5NO]2− (M![]() ![]() ![]() ![]() |
Nanosecond laser flash photolysis experiments were carried out with standard equipment, similar to the one used in previous work,27 consisting of two beams (one for excitation and the other for analysis) crossing each other at 90°, a holder with a 1 cm quartz cuvette and a photomultiplier for detection. A XeCl excimer laser pulse at 308 nm (EMG 101 MSC Lambda Physik) pumped a dye laser (FL 2000 Lambda Physik, pulse length ≈15 ns, 1 Hz repetition rate) in order to have excitation wavelengths near 400 nm. The third harmonic of the Nd:YAG laser at 355 nm was used in some cases. The analysing beam source was a pulsed 150 W Xe arc lamp for the μs range and a continuum halogen lamp for the ms range. Two matched energy heads (Laser Precision RJP 735) connected to a Laser Precision RJ-7100 energy meter or Rm6600 energy ratio meter were used for the monitoring of the laser beam energy. The signal detected by the photomultiplier was fed through a 50 ohm resistor into a Tektronix TDS 520A oscilloscope. The signal, the baseline (no laser), and the scattering signal (no analysing beam) were taken and combined in order to obtain the ΔA values at the various observation wavelengths.
The set-up used for laser-induced optoacoustic spectroscopy (LIOAS) experiments was similar to that previously described.28–31 The pulses from the OPO system described above were used for excitation. The fluence of the pulses was measured with energy meters as described above. The laser beam width was set with a slit (0.5 × 5 height) mm, which allows a time resolution from ca. 20 ns (using deconvolution) up to 5 μs. The sound wave was detected with a PZT ceramic transducer pressed against the sidewall of the cuvette, 100 times amplified, and fed into a signal digitiser (Tektronix 520 A or TDS 744 A). The absorbance of the samples (approximately 0.15, the exact value depending on the experiment) were matched at room temperature within ±0.005 units to those of the calorimetric reference solution (brilliant black). No temperature dependence was detected for the absorption spectra of sample and reference solutions.
The LIOAS signal handling using deconvolution was discussed in several publications.28,29,32 A sum of single-exponential decays fitting function was used for the time-resolved pressure evolution in the medium upon excitation of the sample. The recovered amplitudes (φi) of the fitting function, normalized with respect to the amplitude of the LIOAS signal for the calorimetric reference, are given by eqn. (3):
![]() | (3) |
The thermoelastic parameter ratio, (cpρ/β)T, for the solutions in 0.1 M buffer, was determined by comparing the signal amplitudes of the reference (Hr) in the buffered solution (sol) and in neat water (w), at the same temperature T, according to eqn. (4), as already described.33
![]() | (4) |
![]() | (5) |
![]() | (6) |
[MII(CN)5NO]2−
+
hν
→
[MIII(CN)5(H2O)]2−
+ NO (M = Fe, Ru, Os) | (7) |
In previous work with NP, the quantum yields of the reaction measured through the production of the pentacyanoaquaferrate(III), Φ(FeIII), were shown to be wavelength dependent (0.35 and 0.18 at 366 and 435 nm, respectively).22 Irradiation at 313 nm afforded Φ(FeIII) = 0.37.35 The absorption maxima of NP appear at ca. 510, 400, and 320 nm (Fig. 3).38 A wavelength dependent Φ(NO) (0.20 at 420 nm and 0.32 at 320 nm) was also determined from the rate of decay of nitronyl nitroxide (monitored by ESR spectrometry) produced upon reaction of the photogenerated NO with it.36
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Fig. 3 Absorption spectra of [MII(CN)5NO]2− ions in 0.1 M NaH2PO4/Na2HPO4 buffer. Solid line: M![]() ![]() ![]() ![]() ![]() ![]() |
In the present work, the quantum yields for NO-formation, Φ(NO), for the three [M(CN)5NO]2− complexes were obtained by electrochemically sensing the NO produced upon irradiation at various wavelengths, a technique already employed for the determination of the stoichiometry of the photodecomposition reaction of [Fe(CN)5NO]2− . This is a simple and fast method for the detection of the gas product in the 10−9M scale, allowing measurements at low conversion.39
The three complexes showed a wavelength-dependent value of Φ(NO) (Table 1), the highest values corresponding to the larger photon energies (lower λexc). The yields for NP in Table 1 are closely similar to those reported earlier at similar wavelengths.22 The coincidence of our Φ(NO) values and the Φ(FeIII) as previously determined (see two paragraphs above), in agreement with the stoichiometry in eqn. (7), is remarkable, indicating that the quantum yield for the detachment of NO (as observed by transient absorbance)22,35 is identical to the final time-integrated quantum yield, and supporting the evaluation of Φ(NO) for the Ru- and Os-analogues, particularly for the latter, which displays a very small photoconversion yield.
Sample | T/°C | Φ(NO) 355 nm | Φ(NO) 435 nm |
---|---|---|---|
[Fe(CN)5NO]2− | 20.0 | 0.28 ± 0.04 | 0.18 ± 0.02 |
[Ru(CN)5NO]2− | 20.0 | 0.10 ± 0.01 | 0.03 ± 0.02 |
[Os(CN)5NO]2− | 20.0 | 0.01 ± 0.005 | ≪ 0.01 |
The quantum yields (for each of the used wavelengths) decrease in the order: Φ(NO)(Fe) > Φ(NO)(Ru) ≫ Φ(NO)(Os). These results should be analysed in terms of the nature of the photoactivation process and the subsequent events. By assuming that the ground state in NP can be described as a {FeIINO+} species,22 the initial excited state should contain an electron in a predominantly π*(NO) orbital, with the metal formally as FeIII. According to the spectral assignments for NP, the main photoactive band for NO-release should be that with maximum at 400 nm, assigned to a transition from the strongly bonding dxz and dyz orbitals to the π*(NO) orbital.22 No significant photoactivity was detected by irradiating above 480 nm,22,37 consistent with the assignment of the band at 510 nm to a transition from the nearly non-bonding dxy orbital to the same π*(NO) orbital. This transition should not produce a significant loss in the M–N bond strength upon excitation. The lower value of Φ(NO) at 436 nm may be traced to the simultaneous excitation of both the overlapping photoactive and inactive bands with maxima at 400 and 510 nm, respectively. On the other hand, the larger value of Φ(NO) on irradiation at 366 or 355 nm should be due to the simultaneous excitation of the band with maximum at 400 nm, as well as that with maximum at 320 nm (mainly a d–d transition). As the same Φ(FeIII)35 and a similar Φ(NO)36 were observed for NP on irradiation at 320 nm, we conclude that an efficient population of the species absorbing at 400 nm is achieved also when exciting at shorter wavelengths.
The trends in the quantum yields correlate with the increasing M–N bond strengths and inertness of the heavier metals, as measured by the relative dissociation rates for the three [MII(CN)5L]n− complexes with a given L ligand, namely k−L(Os) ≪ k−L(Ru) < k−L(Fe).40 In the M(III) complexes, the MIII–NO bond is mainly of σ type,41 and then we should also expect an increasing σ-bond strength when going from the Fe to the Os derivative. Thus, the decreasing quantum yields in Table 1 can be rationalized by considering that a rate-controlling M(III)–nitrosyl bond reorganization is the key factor for NO release (see below). However, it must be recognized that the same trend in the quantum yields should also be expected considering the stronger spin–orbit effects when going from Fe to Os. These should favour the non-radiative deactivation routes in competition with the photodetachment of NO.19
Upon excitation at 308 nm the three [M(CN)5NO]2− ions showed a broad emission in the range 300–600 nm, centred around 500 nm, with a half-bandwidth of ca. 5000 cm−1. Some structure could be observed in the emission of [Ru(CN)5NO]2− with shoulders at 470 and 500 nm.
Similar emissions, both in energies and bandwidths, have been detected upon excitation of [Ru(CN)6]4−,42 and of [Fe(CN)5CO]3−.43 These emissions have been assigned to the deactivation of the corresponding d–d states (3T1g and 3A2, respectively). An analogous population of 3A2 states can be also envisioned for [Fe(CN)5NO]2− upon the competitive deactivation of the initially accessible CT state, in view of the similar binding properties of the isoelectronic CO and NO+ ligands.
The trend in the fluorescence quantum yield (Table 2) is opposite to that determined for the Φ(NO) values, suggesting that the primary CT state deactivates competitively (at least upon excitation at 308 nm) into the photochemically active ground state potential energy surface and the emissive d–d state.
Sample | (Φf ± 2) × 103 |
---|---|
[Os(CN)5NO]2− | 8.5 |
[Ru(CN)5NO]2− | 7 |
[Fe(CN)5NO]2− | 3 |
Two additional aspects of the photoreactivity were tested with the Fe(II) complex presenting the highest NO production yield, i.e., changes in temperature and in the medium. Φ(NO) decreased to one third of the original value upon decreasing the temperature from 20 to 0.8 °C (Table 3, Fig. 4). This is consistent with an activated process for an event subsequent to photoexcitation.
Sample | T/°C | Φ(NO) | ||
---|---|---|---|---|
355 nm | 428 nm | 480 nm | ||
[Fe(CN)5NO]2− | 20.0 | 0.28 ± 0.04 | 0.18 ± 0.02 | 0.10 ± 0.02 |
[Fe(CN)5NO]2− | 4.8 | 0.10 ± 0.02 | 0.19 ± 0.02 | 0.04 ± 0.02 |
[Fe(CN)5NO]2− | 0.8 | 0.10 ± 0.02 | 0.14 ± 0.02 | 0.03 ± 0.02 |
[Fe(CN)5NO]2−/[24]ane-N8+ | 20.0 | — | 0.11 ± 0.02 | — |
[Fe(CN)5NO]2−/[32]ane-N8+ | 20.0 | 0.16 ± 0.02 | — | — |
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Fig. 4 NO photodelivery upon excitation of [FeII(CN)5NO]2− at 355 nm in 0.1 M NaH2PO4/Na2HPO4 (pH![]() ![]() |
Regarding the medium changes, the Φ(NO) values proved to be independent of pH (in the 1–7 range).
Nitrogen macrocycles influenced the reactivity. Addition of an excess of 24[ane]-N8H8·8HCl (0.1 M HCl, I = 0.8 M, NaCl) and of 32[ane]-N8H8·HCl (0.1 M HAcO/AcO− buffer, pH 4.5, I = 0.5 M, NaCl) to an NP solution did not change the absorption spectra, but decreased Φ(NO) to almost half of the value in the absence of the macrocycle. This is interpreted in terms of specific (electrostatic and hydrogen bond) interactions between the macrocycle and the cyano groups of the caged compound.44 Proton donation to cyanides should decrease the metal electron density, thus strengthening the σ Fe(III)–nitrosyl bond. In a recent work with a series of cis-[RuL(bpy)2NO]3+ complexes,16 the values of Φ(NO) were shown to decrease for L = 4-picoline > py > 4-acetylpyridine. This is consistent with our argument that the more donor L ligands favour the M(III)–NO bond cleavage.
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Fig. 5 Transient absorption signals for [M(CN)5NO]2−; λexc![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() |
In each case a stable product is formed in less than 1 μs (Fig. 5). The small values of Φ(NO), the spectral overlap between reactant and product, the low absorption coefficients of the product, and the photodecomposition of the parent compound, which hindered the averaging of a large number of traces, determined a very bad signal/noise ratio, and, consequently, impaired a good time resolution. This is probably also the reason why no clear transient absorbance signal was detected for the Os aqua-derivative [electrochemically detected Φ(NO) = 0.16 ± 0.02 upon excitation at 308 nm]. [FeIII(CN)5H2O]2− was already shown to be produced within the resolution of the equipment in the microsecond time range upon pulsed excitation of NP.37
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Fig. 6 LIOAS signals after excitation at 480 nm of solutions of the calorimetric reference and NP in 0.1 M NaH2PO4/Na2HPO4 buffer (pH 6.5) at 4.8 °C, together with the simulation curve (overlapping the thick sample signal) and the residuals distribution. One exponential was used for the fitting with a time constant of 44 ns. |
Upon excitation at 355 nm, deconvolution with one exponential always resulted in a very short production time of < 1 fs, which essentially means that the pressure wave is generated in a time well below the observation window of the experiment. However, since the amplitude of the signal was extremely small at this temperature and wavelength, the lifetimes are not very precise, and should be taken only as an indication of the occurrence of the process.
The LIOAS signals obtained upon excitation at 480 nm were well fitted with a single exponential function with a time constant of (120 ± 40) ns at 0.8 °C and (45 ± 15) ns at 4.8 °C (Table 4). The very small and noisy transient absorption signals (see above) impaired the analysis of the initial formation of [Fe(CN)5H2O]2−.
λexc/nm | T/°C | φ | τ/ns | ΔVe/ml mol−1 | ΔVstr/ml mol−1 | ΔH/kJ−1 mol−1 |
---|---|---|---|---|---|---|
480 | 0.8 | 0.12 ± 0.02 | 120 ± 40 | 0.27 | 8 ± 3 | 190 ± 20 |
4.8 | 1.09 ± 0.05 | 45 ± 15 |
The LIOAS signals after excitation at 480 nm could be analysed in a better manner precisely because the quantum yield for NO release is smaller at this wavelength, i.e., there is a larger heat release from the excited species and the LIOAS signals are larger. Therefore, especially the calculation of the enthalpy change is more reliable with the data obtained after excitation at 480 nm. Additionally, one should consider that at lower wavelengths more heat evolves from radiationless deactivation from upper excited levels, which masks other effects.
The above results tell us that at both temperatures and excitation wavelengths the product formed in less than at most 120 ns (at 0.8 °C, as observed upon excitation at 480 nm) lives longer than about 5 times the pressure integration time (i.e. longer than ca. 600 ns). All data indicate that the product is [Fe(CN)5H2O]2−.
A two-exponential function (not shown) also fitted the data, but produced results non-compatible with the transient absorbance observations, since the shorter lifetime was much longer than the rising time of the transient absorption changes, and the amplitude afforded an enthalpy level much larger than the molar laser energy. The distribution of residuals and the χ2 values with the two-exponential function were not better than with the one-exponential fitting function.
The data taken upon excitation at 480 nm indicates that the production time decreases with temperature upon excitation, i.e., there is an activation process on the way from the excited state to the final product.
The reaction volume change per einstein absorbed calculated with eqn. (5) together with the determined value of (β/cpρ) = 9.2 10−3 ml kJ−1 at 4.8 °C and E(480 nm) = 249.1 kJ mol−1, is ΔVe = (0.27 ± 0.05) ml mol−1.
The LIOAS signals upon excitation at 355 nm do not afford reliable quantitative data (see above), especially because at 0.8 °C they are too small.
The calculated fraction of heat released is α(480) = (0.97 ± 0.07) [eqn. (6)]. In view of the fact that NP shows a fluorescence quantum yield of 3 × 10−3 (Table 3), energy balance considerations readily lead to eqn. (8). The energy provided by excitation (Eλ) should be equal to the sum of the prompt heat released (q) and the energy stored by the produced [Fe(CN)5H2O]2−, i.e., the product of its formation quantum yield [(Φ = Φ(NO), vide supra] and its enthalpy content with respect to the parent compound (ΔH).
E(λ) = q + ΦΔH = αE(λ) + Φ(NO)ΔH | (8) |
Considering the molar excitation wavelength E(480 nm) = 249.1 kJ mol−1, the heat delivered is q = αE(λ) = (241.6 ± 100) kJ mol−1. Thus, with Φ(NO) = 0.04 at 480 nm and 4.8 °C (Table 3) the enthalpy difference between [Fe(CN)5NO]2− and [Fe(CN)5H2O]2− is ΔH = [E(λ) − q]/Φ(NO) = (190 ± 20) kJ mol−1.
The structural volume change upon excitation at 480 nm is ΔVstr = ΔVe/Φ(NO) = (0.27 ± 0.05)/ 0.04 = (8 ± 3) ml mol−1. This structural volume change is concomitant with the appearance in ca. 50 ns at 4.8 °C of the long-lived species. Thus, it should correspond to the volume difference between [Fe(CN)5NO]2− and [Fe(CN)5H2O]2−and is consistent with the sum of an expansion due to the loosening of the water molecules linked via hydrogen bonds to the CN groups upon oxidation of Fe(II) to Fe(III), plus the difference in the partial molar volumes of the released NO from the first coordination sphere into the bulk and the entering water replacing the NO. An expansion due to loosening of the H2O molecules was found for the production of the 3MLCT state upon excitation of ruthenium(II)–bipyridine cyano complexes.28 The result is in quite satisfactory agreement with the recently measured activation volume of 7 ml mol−1 for the dissociation of NO from the [Fe(CN)5NO]3− ion.46 This reaction occurs through a dissociative mechanism, in which the structure of the transition state nearly equals the structure of the products; therefore the comparison between an activation volume and the presently reported reaction volume appears as reasonable.
At this point, it seems appropriate to discuss a work on excited state Raman spectroscopy with the potassium salt of NP.47 By pumping at 406 nm after excitation with 9 ns pulses, a new peak appeared at 1835 cm−1, largely down-shifted with respect to that for the parent compound (N–O stretching in NP, ca. 1940 cm−1). The shift was traced to NO-bending upon excitation, but the consideration of more recent evidence on the formation of NO-linkage isomers upon low-temperature irradiation of NP48 allows us to suggest that similar phenomena could be present within the conditions of the irradiation process at ambient temperature. Thus, the primary excitation product, {M(III)–NO} is likely to rapidly deactivate to the ground state potential energy surface,48 affording the η1-M–ON isomer (the so-called MS1 state, ON = isonitrosyl), probably with an intermediate formation of the η2-side-bound isomer (the MS2 state). The MS1 state should be labile for NO release, consistent with the short times observed for the [Fe(CN)5H2O]2− appearance. This process is most likely activated as demonstrated by the temperature dependence of the [Fe(CN)5H2O]2− appearance times determined by LIOAS, and of the NO quantum yields. Quite relevant to this reinterpretation is the fact that the same value for the N–O stretching mode at 1835 cm−1 has been reported for the now well characterized MS1 linkage isomer of NP.49
Footnote |
† Dedicated to Professor Hiroshi Masuhara on the occasion of his 60th birthday. |
This journal is © The Royal Society of Chemistry and Owner Societies 2005 |