
Web Release Date: December 24,
Enthalpies of Formation of Gas-Phase N3, N3-, N5+, and N5- from Ab Initio Molecular Orbital Theory, Stability Predictions for N5+N3- and N5+N5-, and Experimental Evidence for the Instability of N5+N3-







and

Contribution from the Chemical Sciences Division and Fundamental Sciences Directorate, Pacific Northwest National Laboratory, P.O. Box 999, Richland, Washington 99352, Air Force Research Laboratory, Edwards Air Force Base, California 93524, Loker Hydro-carbon Research Institute, University of Southern California, Los Angeles, California 90089, Department of Chemistry, University of Warwick, Coventry CV4 7AL, West Midlands, U.K., and Department of Chemistry, Spedding Hall, Iowa State University, Ames, Iowa 50011
Received May 27, 2003
Abstract:
Ab initio molecular orbital theory has been used to calculate accurate enthalpies of formation
and adiabatic electron affinities or ionization potentials for N3, N3-, N5+, and N5- from total atomization
energies. The calculated heats of formation of the gas-phase molecules/ions at 0 K are
Hf(N3(2
)) =
109.2,
Hf(N3-(1
+)) = 47.4,
Hf(N5-(1A1')) = 62.3, and
Hf(N5+(1A1)) = 353.3 kcal/mol with an estimated
error bar of ±1 kcal/mol. For comparison purposes, the error in the calculated bond energy for N2 is 0.72
kcal/mol. Born-Haber cycle calculations, using estimated lattice energies and the adiabatic ionization
potentials of the anions and electron affinities of the cations, enable reliable stability predictions for the
hypothetical N5+N3- and N5+N5- salts. The calculations show that neither salt can be stabilized and that
both should decompose spontaneously into N3 radicals and N2. This conclusion was experimentally
confirmed for the N5+N3- salt by low-temperature metathetical reactions between N5SbF6 and alkali metal
azides in different solvents, resulting in violent reactions with spontaneous nitrogen evolution. It is
emphasized that one needs to use adiabatic ionization potentials and electron affinities instead of vertical
potentials and affinities for salt stability predictions when the formed radicals are not vibrationally stable.
This is the case for the N5 radicals where the energy difference between vertical and adiabatic potentials
amounts to about 100 kcal/mol per N5.
The discovery of stable N5+ salts,1,2
This interesting concept and our own interests in such compounds led us to perform a different set of calculations on the stability of these compounds. We have also used high level ab initio molecular orbital theory to address the important question of whether the combination of a stable polynitrogen cation, such as N5+, with a stable polynitrogen anion, such as N3-, can lead to a stable ionic nitrogen allotrope, such as N5+N3-. The stability predictions were made using Born-Haber cycles, a well-established and widely used method10 for evaluating the stability of ionic salts, if reliable values for the lattice energies of the salts, the first ionization potential of the anion, and the electron affinity of the cation are available. This approach also requires an excellent knowledge of the nature and stability of the most likely decomposition products.
A critical prerequisite for such stability calculations is the
use of accurate heats of formation and electron affinities and
ionization potentials. We have developed an approach11 to the
reliable calculation of molecular thermodynamic properties,
notably enthalpies of formation, based on ab initio molecular
orbital theory without using empirical parameters. Our approach
involves an accurate calculation of the total atomization energy
of a molecule and combines this value with known enthalpies
of formation of the atoms to calculate the molecular enthalpy
of formation at 0 K. This method starts with coupled cluster
theory, including a perturbative triples correction (CCSD(T)),12-14
This paper provides a conclusive answer to the question of whether the lattice energies of these salts are sufficient to stabilize them as solids, thus preventing spontaneous electron transfer from the anion to the cation and spontaneous decomposition. Furthermore, for N5+N3-, experimental data are provided in support of our theoretical predictions.
Caution! Reactions of N5+ salts with azide ions are violent and can result in explosions. Therefore, these materials should be handled only on a small scale with appropriate safety precautions (face shield, leather gloves, and protective clothing).
Materials and Apparatus. All reactions were carried out in a Teflon-PFA double U-tube apparatus that consisted of a reaction U-tube, a porous Teflon filter assembly, and a receiver U-tube. Volatile materials were handled on a stainless steel/Teflon-FEP vacuum line.18 Nonvolatile solids were handled in the dry nitrogen atmosphere of a glovebox. Infrared spectra were recorded on a Mattson Galaxy FT-IR spectrometer using dry powders pressed between AgCl windows in an Econo press (Barnes Engineering Co.). Raman spectra were recorded on a Bruker Equinox 55 FT-RA spectrometer using a Nd:YAG laser at 1064 nm and Pyrex melting point capillaries as sample containers.
The N5SbF6 was prepared using our previously reported procedure.2 The CsN3 (Aldrich Chemical Co.) was pretreated with an excess of (CH3)3SiN3 to remove any traces of moisture. The SO2 (Air Products) was used as received.
Reactions of N5SbF6 with CsN3. In a typical experiment, N5SbF6
(2.285 mmol) and CsN3 (2.267 mmol) were loaded in the drybox into
a Teflon-PFA reaction vessel that was closed by a Teflon valve. On
the vacuum line, anhydrous SO2 (5.0 mL, liquid) was added at -196
C. The reaction mixture was warmed to the melting point of SO2 (-64
C). After the SO2 had partially melted and the slurry of reactants was
gently agitated, a violent reaction took place producing a bright yellow
flame. The reactor was quickly quenched with liquid nitrogen. A check
for noncondensable gases at -196
C revealed 9.05 mmol of N2 as
expected for the complete decomposition of 2.267 mmol of N5N3 to
N2. Pumping off all volatiles at -64
C produced 0.8890 g of a white
solid residue (weight expected for 2.267 mmol of CsSbF6 = 0.836 g).
The extra weight was due to some residual SO2. Raman and infrared
spectra of the white solid, after pumping at room temperature, showed
it to be pure CsSbF6.
This reaction can be moderated by the separate dissolution of the
starting materials in SO2 and the combination of the resulting clear
solutions at -64
C. Under these conditions, the decomposition reaction
proceeded rapidly but without violence and gave the same results as
described above.
Reactions of N5SbF6 with NaN3. To equimolar amounts of NaN3
and N5SbF6 was added CHF3 as a solvent at -196
C, and the resulting
mixture was warmed to -95
C and then to -64
C. No N2 evolution
was observed under these conditions. The CHF3 was pumped off at
-95
C, and SO2 was added as a solvent at -196
C. The mixture
was warmed to -64
C, but again no N2 evolution was observed.
Pumping off the SO2 at -64
C resulted in a white solid residue that,
based on its room-temperature Raman spectrum, consisted of a mixture
of unreacted NaN3 and N5SbF6, indicating that no reactions had occurred
due to the very low solubility of NaN3 in these solvents.
Enthalpies of Formation. The augmented correlation consistent
basis set aug-cc-pVnZ (n = D, T, Q)19 was used for nitrogen. Only the
spherical components (5-d, 7-f, 9-g and 11-h) of the Cartesian basis
functions were used. This family of basis sets contains an additional
shell (e.g., spd for DZ) of diffuse functions that are necessary for an
accurate description of anions. Calculations were performed using the
MOLPRO,20 Gaussian,21 and GAMESS22 suites of programs. The open
shell CCSD(T) calculations were carried out at the R/UCCSD(T) level.
In this approach, a restricted open shell Hartree-Fock (ROHF)
calculation was initially performed to generate the set of molecular
orbitals and the spin constraint was relaxed in the coupled cluster
calculation.23-25
with n = 2 (aug-cc-pVDZ), 3 (aug-cc-pVTZ), etc., as first proposed
by Peterson et al.26 This extrapolation method has been shown to yield
atomization energies in the closest agreement with experiment by a
small measure as compared to other extrapolation approaches up
through n = 4.8
Most geometries were optimized at the frozen core CCSD(T) level with various augmented correlation-consistent basis sets. With the exception of the N5 radical, all geometries were optimized with the aug-cc-pVTZ or aug-cc-pVQZ basis sets. If the CCSD(T)/aug-cc-pVQZ geometry was not available, the CCSD(T)/aug-cc-pVTZ geometry was used for the CCSD(T)/aug-cc-pVQZ calculation. Geometries for the N5 radicals were obtained from ZAPT2/6-311+G(2df) and CCSD(T)/aug-cc-pVDZ calculations. Vibrational frequencies were calculated at the CCSD(T) and MP2 levels with the aug-cc-pVDZ basis set. Calculations were performed on SGI, IBM, and Apple G4 computers.
Core-valence corrections,
ECV, were obtained at the CCSD(T)/cc-pCVTZ level of theory.27 Scalar relativistic corrections (
ESR), which
account for changes in the relativistic contributions to the total energies
of the molecule and the constituent atoms, were included at the CI-SD
(configuration interaction singles and doubles) level of theory using
the cc-pVTZ basis set.
ESR is taken as the sum of the mass-velocity
and 1-electron Darwin (MVD) terms in the Breit-Pauli Hamiltonian.28
Because N has a 4S ground state, there are no atomic spin-orbit
corrections to the total atomization energies. The spin-orbit coupling
constant for N3 is 71.3 cm-1 based on experiment,29 leading to a spin-orbit correction of 0.10 kcal/mol.
By combining our computed
D0 values with the known enthalpies
of formation30
Hf0(N) = 112.53 ± 0.02 kcal mol-1,
we can derive
Hf0 values for the molecules under study in the gas
phase. We obtain enthalpies of formation at 298 K by following the
procedures outlined by Curtiss and co-workers16 and by using the
stationary electron convention; that is, we do not assume a change in
the enthalpy of formation of the electron as a function of temperature.
Lattice Energies. For this study, eq 231

and
take the values 28.0 kcal mol-1 nm and 12.4
kcal mol-1, respectively, for 1:1 salts. The individual ion volumes can
be estimated from an ion volume database,31 inferred in some cases
from established crystal structure data, or calculated. To calculate the
volumes of the ions, we chose to use the volumes that we have used
in free energy of solvation calculations.32 The electron densities were
calculated at the B3LYP/6-31+G* level,33 and the volume was taken
to be that inside the 0.001 au contour of the electron density.
Calculated Geometries. The calculated geometries for the
molecules, N2, N3, N3-, N5-, and N5+ are summarized in Table
1
.
N2. As expected, the geometry for N2 at the CCSD(T)/aug-cc-pVQZ level is in excellent agreement with the experimental value.34 Theory overestimates experiment by 0.0028 Å. For comparative purposes, we also optimized the N-N bond length with the larger aug-cc-pV5Z basis set. This produced a small 0.0010 Å decrease in the bond length, indicating that the aug-cc-pVQZ bond lengths should be within approximately 0.001 Å of the basis set limit for the other molecules that could be treated at this level of theory. If the frozen core approximation is removed via calculations with the core/valence (CV) cc-pCVQZ basis set, another 0.0020 Å shortening of the bond length is observed. The final CCSD(T)/aug-cc-pV5Z + CV bond length of 1.0975 Å is almost identical to the experimental value of 1.0977 Å.
N3. The geometry for N3 (D
h) is in excellent agreement with
the experimental value.35 The calculations predict a value for
the NN bond that is slightly shorter than the experimental value.
This result is in contrast to N2 where the calculations predict a
longer bond at the CCSD(T)/aug-cc-pVQZ level.
N3-. The calculated geometry for N3- is also in very good agreement with experiment, with the calculated NN bond length again being slightly shorter than experiment.36
N5+. The geometry for N5+ has been measured in the crystal by X-ray diffraction techniques.2 The calculated values are in good agreement with the crystal structure values considering the uncertainty in the experimental values and the different environment. The calculated geometrical parameters for N5+ are the same as those reported by Fau and Bartlett at the CCSD(T)/aug-cc-pVTZ level,5 whereas the geometries calculated for N3- at the same level differ slightly.
N5-. The value of 1.334 Å calculated for the NN bond length in N5- at the CCSD(T)/6-311+(G(d,p) level7 lies between our values calculated at the CCSD(T) level with the aug-cc-pVDZ and aug-cc-pVTZ basis sets, respectively.
N5 (Open Isomer). ZAPT237 calculations with the 6-311+G(2df) basis set followed by CCSD(T)/cc-pVTZ single-point
calculations confirm previous conclusions7 that the N5 radical
starting from this geometry is vibrationally unstable. Starting
N5 (Cyclic Isomer). The N5 radical cyclic isomer would be
generated by detaching an electron from cyclic N5-. The HOMO
of N5- is a degenerate in-plane orbital involving essentially lone
pair interactions. Production of the N5 radical leads to (e)3
occupancy which Jahn-Teller distorts to a C2v structure. Two
states can be derived from the (e)3 occupancy, a 2A1 state and
a 2B1 state (a 2B2 state would be a
radical). The geometry for
the cyclic N5 (C2v) 2A1 radical was found to be a stationary
point on the ZAPT2/6-311+G(2df) potential energy surface. The
cyclic N5 radical at the ZAPT2/6-311+G(2df) geometry is 66.8
kcal/mol above the N3 + N2 asymptote at the CCSD(T)/cc-pVTZ level. The longest NN ZAPT/6-311+G(2df) bond
distance is that in the base of the pentagon, 1.354 Å. The shortest
NN bonds are those connected to the apex, 1.292 Å. We took
this geometry and initiated an optimization at the R/UCCSD(T)/aug-cc-pVDZ level for both the 2A1 and the 2B1 states under
the constraint of C2v symmetry. The 2B1 state smoothly
dissociated to the N3 + N2 asymptote, showing that on the
CCSD(T)/aug-cc-pVDZ surface, this state is not a minimum.
The N3 distance converges faster than the N2 distance. The 2A1
state is difficult to optimize but finally optimizes to a structure
with two elongated N2 molecules complexed weakly to an N
atom (see Table 1), as it cannot go to the products N2 + N3. At
the CCSD(T)/aug-cc-pVTZ level using the optimized CCSD(T)/aug-cc-pVDZ geometry, the 2A1 state is 60.2 kcal/mol above
the N2 + N3 asymptote. These calculations strongly suggest that,
on electron detachment from N5-, the resulting radical has a
path on the 2B1 surface that leads directly to the N3 + N2
asymptote and that there is no stable cyclic N5 radical structure,
as has already been noted previously.7 As part of a study of
Fe(
5-N5)2, Frenking and co-workers reported a structure for
the 2A1 state of the N5 radical at the B3LYP/6-31G(d) level
which could be a minimum, although the structure was not
discussed.38 Our result is also consistent with the prediction7
of Nguyen and Ha that cyclic N5 is not stable with respect to
dissociation.
Calculated Frequencies. The calculated vibrational frequencies for N2, N3, N3-, N5-, N5 (cyclic), and N5+ are summarized
in Table 2
.
N2. The harmonic frequency at the frozen core CCSD(T)/aug-cc-pVQZ level is within 5 cm-1 of the experimental value.34
Even at the CCSD(T)/aug-cc-pVTZ level, the N2 frequency is
within 20 cm-1, and, at the CCSD(T)/aug-cc-pVDZ level, it is
within 40 cm-1. This level of agreement is in part fortuitous.
Whereas the aug-cc-pV5Z basis set frequency is identical to
the experimental value, introduction of core/valence correlation
increases
e by 9.2 cm-1. Thus, the final CCSD(T)/aug-cc-pV5Z
+ CV value is 9 cm-1 larger than experiment.
N3. For N3, the frequencies calculated at the MP2/aug-cc-pVDZ level are in qualitative agreement with the experimental
values39 for the
bend and the symmetric stretch and in good
agreement for the antisymmetric stretch. In this case, we have
used the experimental frequencies to calculate the zero-point
energy.
N3-. For N3-, the calculated antisymmetric harmonic stretch
is in excellent agreement with the gas-phase experimental
value.35,40 The value for the
2 bending frequency for this ion
has been measured in the solid state, and a free space estimate
for
1 has been obtained based on the spectrum measured for
the solid.41,42
1 and
3 are in reasonable agreement with those
previously calculated at the CASPT2 level17 and at the CEPA
level.42
N5-. For this ion, we used the frequencies calculated at the CCSD(T)/aug-cc-pVDZ level for the zero-point energy calculation as there are no experimental values available. Quite good agreement is found for the frequencies of N5- calculated at the MP2/aug-cc-pVDZ level and at the CCSD(T)/aug-cc-pVDZ level. The CASPT2 frequencies17 are similar to our values.
N5 (Cyclic Isomer). Frequencies were calculated at the ZAPT2/6-311+G(2df)level of theory for the 2A1 state. No experimental values are available for this species. As noted above, the 2B1 structure is not a minimum for the cyclic radical at the R/UCCSD(T)/aug-cc-pVDZ level.
N5+. For N5+, there is reasonable agreement between the frequencies calculated at the MP2/aug-cc-pVDZ level and the average of the frequencies taken from measurements in the solid state.2 The largest discrepancy is found for the highest frequency b2 mode with a difference of ~140 cm-1. The calculated a2 and b1 modes deviate by ~50 cm-1 from the experimental values. The fact that the differences cancel out leads to calculated and experimental zero-point energies that are essentially identical. We used the average experimental values in our zero-point energy calculations. Our calculated frequencies are in qualitative agreement with those calculated at the CCSD(T)/6-311+G(2d) and B3LYP/6-311+G(2d) levels.1,2 The CCSD(T) values are in general lower than our MP2 values except for the a2 and b1 modes which are higher. The CASPT2 frequencies differ from ours more than might be expected, especially for the two highest modes.17
Calculated Enthalpies of Formation. The total atomization
energies are given in Table 3
. The
Hf0 values were converted
to 298 K following the procedure of Curtiss and co-workers.16
N2. As shown in Table 3, the error in the atomization energy of N2 is 0.76 kcal mol-1 when compared to experiment.30 This leads to an error in the calculated enthalpy of formation at 0 K of 0.76 kcal mol-1. We can thus estimate that the error bars in our heats of formation are likely to be on the order of ±1 kcal/mol.
N3. The enthalpy of formation of N3 has been reported by a
number of authors. The NIST value30 of 100 ± 5 kcal mol-1 at
0 K is almost 10 kcal mol-1 below our calculated value. Our
calculated value of 109.2 kcal mol-1 is in much better agreement
with the value of 112 ± 5 based on the experimental measurement of the acidity of HN3 and the measurement of the electron
affinity of N3-.43,44
is only 4 kcal mol-1 endothermic at 0 K.
N3-. The enthalpy of formation of N3- has been determined from gas-phase acidity measurements and the enthalpy of formation of HN3 to be 48 ± 2 kcal mol-1.43 This value is in excellent agreement with our calculated value of 47.2 kcal mol-1. Fau and Bartlett calculated the enthalpy of formation of N3- by a variety of methods.5 Their best estimated enthalpy of formation of 47.8 kcal mol-1 is in good agreement with our value. The electron affinity of N3 has been measured to be 2.68 ± 0.01 eV.44 Our calculated adiabatic electron affinity of 2.69 eV is in excellent agreement with this result. With an ANO (4s3p2d1f) basis set, the CASPT2 electron affinity was predicted to be 2.64 eV.17
N5+. The enthalpy of formation of N5+, calculated by us, is
353.4 kcal mol-1. This result is in reasonable agreement with
the value of 347.1 kcal mol-1, calculated by Fau and Bartlett.5
Christe and co-workers1,2 predicted the enthalpy of formation
of N5+ to be 351.1 kcal mol-1 at the CCSD(T) level with a
polarized double-
basis set. Nguyen and Ha predict a heat of
formation of 351.3 ± 3.6 kcal/mol based on CCSD(T)/6-311+
G(3df) calculations and the experimental energy of N3.7
The adiabatic electron affinity of N5+ is given by the energy
difference between its enthalpy of formation and those of the
first metastable neutral reaction or decomposition products.
Because the intermediate, open-chain N5 radical, formed by the
addition of an electron to N5+, is unstable and spontaneously
dissociates to N3 (g) + N2 (g), the energy of reaction 4 provides
the adiabatic electron affinity of N5+.

N5-. The enthalpy of formation of N5- is calculated to be
62.2 kcal mol-1, in excellent agreement with the value of 62.1
± 3.6 kcal/mol given by Nguyen and Ha.7 This value can be
used to calculate the adiabatic ionization potential of N5- in
the same manner as discussed above for N5+. As noted above,
loss of an electron from the degenerate HOMO of N5- leads to
either a 2B1 or a 2A1 radical. We have shown that formation of
the 2B1 radical provides a pathway leading to N3 + N2, so the
following channel (reaction) represents the adiabatic ionization
process:

The important dissociation channel for N5- is the formation of N3- + N2. We predict this channel to be exothermic by 14.2 kcal mol-1 at 0 K. This value is in good agreement with the value of 14.3 kcal mol-1 reported by Nguyen and Ha at the CCSD(T)/aug-cc-pVTZ level.7 It is important to know if there is a barrier separating N5- from the asymptotic products N3- and N2. Nguyen and Ha calculated the energy barrier to dissociation as 27.7 kcal mol-1 at the CCSD(T)/aug-cc-pVTZ level including zero-point corrections based on a geometry calculated at the CCSD(T)/6-311+G(d) level.7 We have calculated the energy of the transition state at the CCSD(T)/CBS level with Nguyen and Ha's geometry and with the geometry optimized by us at the MP2/aug-cc-pVDZ level. We calculated the geometry at the latter level to get a value of the zero-point energy as well as the value of the imaginary frequency characterizing the transition state. The results are given in Tables 1-3. Our calculated energy barrier using the MP2 geometry is 29.4 kcal mol-1, and when the zero-point energy difference is included, the barrier is 27.2 kcal mol-1. The energy barrier using the Nguyen and Ha geometry is 0.61 kcal mol-1 higher in energy than our value based on the MP2 geometry, showing that the two geometries give essentially identical barrier heights. The barrier calculated7 by Nguyen and Ha is very similar to our CCSD(T)/CBS value using their geometry. At the CASPT2/ANO(4s3p2d) level, the barrier is predicted to be 26 kcal mol-1, and the dissociation energy to N3- and N2 is predicted to be exothermic by 9 kcal mol-1,17 5 kcal mol-1 lower than our value. A calculation of the imaginary frequency for the transition state of the N5- decomposition shows a large value of 862i cm-1, suggesting that the ion might be able to tunnel through the barrier to reach the products. We can make a crude estimate of the tunneling effect by using the Wigner expression.45 This leads to an enhancement of the dissociation rate by 1.7 at 298 K. This suggests that tunneling should be considered when predicting the stability of N5-. For lower temperatures, a larger tunneling effect would be expected.
The origin of the difference between the vertical and the adiabatic potentials, of course, is the dissociation energy of neutral N5 to N3 and N2. Vertical electron affinities or ionization potentials for the ionic systems under study correspond to removal or addition of an electron to the ion to form a radical at the geometry of the ion. Only when the neutral radicals are vibrationally stable species with geometries similar to those of the starting materials will their vertical EA or IP values approximate the adiabatic values. If this is not the case, the radicals generated by the neutralization process spontaneously undergo further decomposition. If these decompositions to the first well-defined, vibrationally stable products do not involve any significant activation energy barriers and if they occur on a fast time scale, it is appropriate to add their energies to the vertical potentials.
Lattice Energy Calculations. Prediction of lattice energies, UL, based on eq 2 requires an estimate of the relevant ion volumes and gives the following results:
N5+N3-. V(N5+) is estimated to be 0.051 (±0.020) nm3 based on the reported2 crystal structure volume for N5+Sb2F11- by subtraction of V(Sb2F11-) (Table 6, ref 31). V(N3-) is equal to 0.058 (±0.014) nm3 (Table 5, ref 31), and thus V(N5+N3-) = 0.109 (±0.024) nm3, leading to an estimate for UL(N5+N3-) = 142 (±7) kcal mol-1.
N5+N5-. An upper limit for V(N5-) can be estimated from
consideration of V(N2) and V(N3-). The volume of solid
dinitrogen, V(N2), which is dimorphous,46 can be obtained from
crystal structure data for the
-cubic and the hexagonal forms
and averages to V(N2) = 0.046 (±0.001) nm3, leading to
V(N5+N5-) = 0.155 (±0.014) nm3, giving a value for UL(N5+N5-)
= 129 (±5) kcal mol-1. Alternatively, we can estimate the
volume of the ions at the B3LYP/6-31+G* level as described
above: V(N5+) = 0.068 nm3; V(N5-) = 0.088 nm3, V(N3-) =
0.065 nm3. These estimated volumes yield UL(N5+N5-) = 129
kcal mol-1 and UL(N5+N3-) = 135 kcal mol-1, well within the
above error limits. The corresponding lattice enthalpies,
HL,
appropriate for use in the cycles of Figures 2 and 3 are
UL(N5+N5-) + 2RT and UL(N5+N3-) + 3/2RT, respectively.
Stability Predictions Based on Born-Haber Cycles. For
a chemical reaction to be thermodynamically favorable, its free
energy change must be zero or negative. If the reaction involves
a barrier, a sufficient amount of activation energy must be
supplied to overcome this barrier. If the reaction does not have
an activation energy barrier, a spontaneous reaction occurs when
its free energy change becomes negative. An example of such
a reaction is the dissociation of an ionic solid into two radicals
(reaction 6), assuming that the electron transfer from the cation
to the anion proceeds without a barrier.



S term to the free energy
must also be included. For the reactions considered in this paper,
these contributions are always negative. We can estimate the
entropy changes for reactions 7 and 8 as follows. The entropy
for the solid is not known, but we can use the entropies of
NH4+NO3- and NH4+N3-, which are 36 and 27 cal/mol K,47
respectively, to estimate the value for the N5+ salts. Given the
well-established entropies of N2 and N3 of 45.8 and 54.1 cal/mol K, respectively, we obtain at 298 K for reaction 7 -T
S
= -49 kcal/mol, if the entropy of NH4+NO3- is used to estimate
that of the solid, and -T
S = -51 kcal/mol, if the entropy of
NH4+N3- is used. For reaction 8, the respective values are -T
S
= -35 and -38 kcal/mol at 298 K. Thus, significantly positive
reaction enthalpy values would be required for the compensation
of the large negative entropy contributions and the stabilization
of N5+N5- and N5+N3-. A positive
Gr value represents the
minimum dissociation energy barrier, but one should keep in
mind that the actual barrier can well be higher. If, however, the
Gr change is negative, spontaneous decomposition occurs in
the absence of a significant reaction barrier. The potential energy
curves for both scenarios are depicted in Figure 4 for N5+N5-.
The left curve of Figure 4 represents the case of the enthalpy
of reaction 7 being negative and having no significant activation
energy barrier. It results in spontaneous decomposition of the
solid to the first vibrationally stable intermediates, that is, N3
radicals and N2. The right curve of Figure 4 represents the
scenario of a positive reaction enthalpy, the only condition under
which solid N5+N5- might exist. This, however, is a hypothetical
case, requiring the enthalpy of formation of N5+N5- to be about
100 kcal mol-1 more negative than the calculated value. Because
the values for the IP of N5- and the EA of N5+ are fixed, the
lattice energy of N5+N5- would have to be about 100 kcal/mol
higher than our calculated value, which is impossible based on
the molar volumes of the ions involved. The relatively small
uncertainties in our
Hr values, -65 ± 7 kcal mol-1 for N5+N5-
and -39 ± 9 kcal mol-1 for N5+N3-, together with the large
-T
S terms, allow us to predict with confidence that both
compounds cannot be stabilized in the form of ionic solids.
The potential energy surface for N5+/N5- is quite complicated. The asymptotic energy of N5+ + N5- is 416 kcal/mol above that of 5N2 molecules at 0 K. Our approach to the ion pair energy provides an estimate of 297 kcal/mol above 5N2, in good agreement with the Fau et al.6 value of 296 kcal/mol. The highly endoergic heat of formation means that the complex is metastable as are all polynitrogen compounds. Thus, there may be a number of decomposition paths.48 Neither the N5 radical derived from N5+ at the cation geometry nor the N5 radical derived from N5- at the anion geometry are stable species as shown above. These two N5 species are doublets, and hence there can be both a triplet coupling and a singlet coupling of the two unpaired electrons after the electron transfer process. The singlet coupling, if the geometries remain similar to the parent ion geometries, should generally be considered as an open shell singlet, not necessarily restricted to a closed shell description.6 Enforcing singlet closed shell (i.e., RHF) pairing in the ground-state wave function prevents the two N5 species from coming apart as N5 radicals (or their dissociative products N2 and N3) even though the product formation of 2N3 + 2N2 is more than 80 kcal/mol exothermic. On the other hand, the triplet surface could lead to direct dissociation. Including the open shell-singlet paired configuration in a more general multiconfigurational wave function may have the same result. To further study the N5+/N5- ion pair potential surface, we optimized the lowest 3A' and 3A' ' states at the ROHF/6-31+G(d) (restricted open shell Hartree-Fock) level, and the lowest 1A' and 1A' ' states using TCSCF (two-configuration self-consistent field) wave functions and the same 6-31+G(d) basis set. For both spin states, the lower energy state is A'. Geometry optimization of the 3A' state (lowest energy triplet at this level of theory) leads to a large separation of the anion and cation, with a concomitant decrease in the charges on the two species to nearly zero. So, the lowest energy triplet is clearly on its way to dissociation to two radicals, and subsequently to N2 and N3. The other three states (two singlets and one triplet) do not appear to dissociate at these levels of theory. The 3A' state is about 40 kcal/mol above the 1A' state but is still ~80 kcal/mol below the separated ion pair dissociation asymptote, showing that there is an electron transfer step leading to dissociation that occurs significantly below the energy of the separated ions. Higher levels of theory may alter these results, and we did not further explore the barriers to dissociation. These results and those of other workers do show that the potential energy surface is very complicated and that there are many potential highly exothermic paths leading to formation of N3 and/or N2. In addition, we note that all of these comparisons are at 0 K and that at higher temperatures, there is a significant entropic effect favoring formation of N2 and N3. These results are all consistent with our conclusion that formation of a stable N5+/N5- ion pair is unlikely, so it cannot be isolated.
Experimental Results and their Comparison with the
Predictions. All of our attempts to prepare solid N5+N3- by
the metathesis reaction 9 failed.

C = 3.14 × 10-3 mol mL-1) CsN3,
violent reactions occurred resulting in quantitative formation
of poorly soluble (solubility at -64
C = 6.56 × 10-6 mol
mL-1) CsSbF6 and 4N2. Using poorly soluble (solubility at -64
C = 9.23 × 10-5 mol mL-1) NaN3, the metathesis did not
proceed to any measurable extent, and unreacted NaN3 and N5SbF6 were recovered. It was also shown that solid NaN3 and
N5SbF6 can be mixed as dry powders at room temperature and
the Raman spectrum of the mixture can be recorded without
evidence of reaction provided that the laser power is kept at a
low level. Attempts to carry out the metathesis in CHF3 solution
were also unsuccessful because of the low solubility of the
starting materials in this solvent. These experiments show that,
in all cases where metathesis took place, only spontaneous
decomposition was observed and, thus, confirm the above given
theoretical predictions.
These results are consistent with the predictions by us and by Fau and Bartlett5 that N5+N3- will not be stable. Fau and Bartlett5 noted that the reaction of N5+ and N3- does not lead to ion pair formation and that N5N3 is a weak complex even on the closed shell singlet energy surface. This structure is located at -149 kcal/mol on the way toward the 2N3 + N2 final products at -182 kcal/mol (energies with respect to the separated ions). Their results suggest that on the triplet coupled surface, and possibly on the multiconfigurational singlet surface, this species will fully dissociate.
Assessment of the Performance of Solid N5+N5- as a
Monopropellant. It was recently suggested6,52
the maximum energy density of N2H4 would be only 1.17 kcal/g.30 The actual value, however, is even lower because there is
always some decomposition of NH3 to N2 and H2.53 Hence, we
conclude that the energy densities of N5+N5- and N2H4 differ
by a factor of 2. Based on our molar volume estimates, the
density of N5+N5- is expected to be 1.50 g/cm3. Even so, we
agree with the conclusion6 that a hypothetical polynitrogen
compound, such as N5+N5-, would be an excellent monopropellant for rocket propulsion or explosives, if it could be
synthesized in a stable form.
The following conclusions can be drawn from our studies:
(i) Our results quantitatively examine the stability of N5+N5- and N5+N3- and show that both compounds are unstable in the solid state.
(ii) Our results show that for Born-Haber cycle based stability estimates for species, such as N5+ and N5-, which decompose to vibrationally unstable species upon neutralization, it is important to use adiabatic ionization potentials and electron affinities.
(iii) In view of the instability of the N5 radicals and their strongly exothermic spontaneous decompositions to N3 radicals and N2, both N5+ and N5- are not good choices for preparing a stable ionic nitrogen allotrope.
(iv) Our results suggest that N5+N5- would be even more unstable than N5+N3-, because the former would contain two unstable N5 species after transfer of the electron.
(v) Stability calculations for individual ions or ion pairs may not provide sufficient information for stability predictions. Rigorous Born-Haber cycles, including realistic lattice energy estimates, and an evaluation of the stability of the decomposition products are required to make meaningful predictions.
(vi) Our theoretical predictions concerning the instability of N5+N3- and the use of the adiabatic electron affinities and ionization potentials are confirmed by extensive experimental studies involving the low-temperature metatheses of N5+SbF6- with different alkali metal azides in various solvents and the determinations of electron affinities by bracketing methods, respectively.
The authors thank Dr. Jerry Boatz for many helpful discussions and Dr. Chang-guo Zhan for help with the volume calculations. The work at Pacific Northwest National Laboratory (PNNL) was supported in part by the U.S. Department of Energy, Offices of Basic Energy Sciences, Division of Chemical Sciences, and Biological and Environmental Research, under Contract No. DE-AC06-76RLO 1830 for PNNL. Part of this research was performed in the William R. Wiley Environmental Molecular Sciences Laboratory (EMSL) at the PNNL using the Molecular Sciences Computing Facility. The EMSL is a national user facility funded by the Office of Biological and Environmental Research in the U.S. Department of Energy. PNNL is a multiprogram national laboratory operated by Battelle Memorial Institute for the U.S. Department of Energy. The work at the Air Force Research Laboratory was supported by the Defense Advanced Projects Agency (DARPA) and the Air Force Office of Scientific Research (AFOSR). The work at the University of Southern California was funded by DARPA, AFOSR, and the National Science Foundation. The work at Iowa State University was funded by an AFOSR high energy density matter (HEDM) grant.
* In papers with more than one author, the asterisk indicates the name of the author to whom inquiries about the paper should be addressed.
PNNL.
AFRL.
USC.
University of Warwick.
Iowa State University.
1. Christe, K. O.; Wilson, W. W.; Sheehy, J. A.; Boatz, J. A. Angew. Chem.,
Int. Ed. 1999, 38, 2004.![]()
2. Vij, A.; Wilson, W. W.; Vij, V.; Tham, F. S.; Sheehy, J. A.; Christe, K. O.
J. Am. Chem. Soc. 2001, 123, 6308.![]()
3. Curtius, T. Ber. Dtsch. Chem. Ges. 1890, 23, 3023.
4. Vij, A.; Pavlovich, J. G.; Wilson, W. W.; Christe, K. O. Angew. Chem.,
Int. Ed. 2002, 41, 3051.![]()
5. Fau, S.; Bartlett, R. J. J. Phys. Chem. A 2001, 105, 4096.![]()
6. Fau, S.; Wilson, K. J.; Bartlett, R. J. J. Phys. Chem. A 2002, 106, 4639.
7. Nguyen, M. T.; Ha, T.-K. Chem. Phys. Lett. 2001, 335, 311.
Nguyen, M.
T.; Ha, T.-K. Chem. Phys. Lett. 2000, 317, 135.![]()
8. Martin, J. M. L.; Francois, J. P.; Gijbels, R. J. Chem. Phys. 1990, 93, 4485.![]()
9. Gagliardi, L.; Orlandi, G.; Evangelsti, S.; Roos, B. O. J. Chem. Phys. 2001,
114, 10733.![]()
10. Greenwood, N. N.; Earnshaw, A. Chemistry of the Elements, 2nd ed.; Butterworth-Heinemann: Oxford, 1998; p 82.
11. Peterson, K. A.; Xantheas, S. S.; Dixon, D. A.; Dunning, T. H., Jr. J. Phys.
Chem. A 1998, 102, 2449.
Feller, D.; Peterson, K. A. J. Chem. Phys. 1998,
108, 154.
Dixon, D. A.; Feller, D. J. Phys. Chem. A 1998, 102, 8209.
Feller, D.; Dixon, D.
A. J. Phys. Chem. A 1999, 103, 6413.
Feller, D. J. Chem. Phys. 1999, 111,
4373.
Feller, D.; Dixon, D. A. J. Phys. Chem. A 2000, 104, 3048.
Feller, D.; Dixon, D. A.
J. Chem. Phys. 2001, 115, 3484.
Dixon, D. A.; Feller, D.; Sandrone, G. J.
Phys. Chem. A 1999, 103, 4744.
Ruscic, B.; Feller, D.; Dixon, D. A.;
Peterson, K. A.; Harding, L. B.; Asher, R. L.; Wagner, A. F. J. Phys. Chem.
A 2001, 105, 1.
Ruscic, B.; Wagner, A. F.; Harding, L. B.; Asher, R. L.;
Feller, D.; Dixon, D. A.; Peterson, K. A.; Song, Y.; Qian, X.; Ng, C.; Liu,
J.; Chen, W.; Schwenke, D. W. J. Phys. Chem. A 2002, 106, 2727.![]()
12. Purvis, G. D., III; Bartlett, R. J. J. Chem. Phys. 1982, 76, 1910.![]()
13. Raghavachari, K.; Trucks, G. W.; Pople, J. A.; Head-Gordon, M. Chem.
Phys. Lett. 1989, 157, 479.![]()
14. Watts, J. D.; Gauss, J.; Bartlett, R. J. J. Chem. Phys. 1993, 98, 8718.![]()
15. Dunning, T. H., Jr. J. Chem. Phys. 1989, 90, 1007.![]()
16. Kendall, R. A.; Dunning, T. H., Jr.; Harrison, R. J. J. Chem. Phys. 1992,
96, 6796.![]()
17. Curtiss, L. A.; Raghavachari, K.; Redfern, P. C.; Pople, J. A. J. Chem.
Phys. 1997, 103, 1063.
18. Christe, K. O.; Wilson, W. W.; Schack, C. J.; Wilson, R. D. Inorg. Synth.
1986, 24, 39.![]()
19. Woon, D. E.; Dunning, T. H., Jr. J. Chem. Phys. 1993, 98, 1358.![]()
20. MOLPRO is a package of ab initio programs. Werner, H. J.; Knowles, P. J.; Almlof, J.; Amos, R. D.; Berning, A.; Cooper, D. L.; Deegan, M. J. O.; Dobbyn, A. J.; Eckert, F.; Elbert, S. T.; Hampel, C.; Lindh, R.; Lloyd, A. W.; Meyer, W.; Nicklass, A.; Peterson, K. A.; Pitzer, R. M.; Stone, A. J.; Taylor, P. R.; Mura, M. E.; Pulay, P.; Schütz, M.; Stoll, H.; Thorsteinsson, T. MOLPRO; Universität Stuttgart and University of Birmingham: Stuttgart, Germany and Birmingham, England, 2000.
21. Frisch, M. J.; Trucks, G. W.; Schlegel, H. B.; Scuseria, G. E.; Robb, M. A.; Cheeseman, J. R.; Zakrzewski, V. G.; Montgomery, J. A.; Stratmann, R. E.; Burant, J. C.; Dapprich, S.; Millam, J. M.; Daniels, A. D.; Kudin, K. N.; Strain, M. C.; Farkas, O.; Tomasi, J.; Barone, V.; Cossi, M.; Cammi, R.; Mennucci, B.; Pomelli, C.; Adamo, C.; Clifford, S.; Ochterski, J.; Petersson, G. A.; Ayala, P. Y.; Cui, Q.; Morokuma, K.; Malick, D. K.; Rabuck, A. D.; Raghavachari, K.; Foresman, J. B.; Cioslowski, J.; Ortiz, J. V.; Stefanov, B. B.; Liu, G.; Liashenko, A.; Piskorz, P.; Komaromi, I.; Gomperts, R.; Martin, R. L.; Fox, D. J.; Keith, T.; Al-Laham, M. A.; Peng, C. Y.; Nanayakkara, A.; Gonzalez, C.; Challacombe, M.; Gill, P. M. W.; Johnson, B.; Chen, W.; Wong, M. W.; Andres, J. L.; Gonzalez, A. C.; Head-Gordon, M.; Replogle, E. S.; Pople, J. A. Gaussian 98, revision A.6; Gaussian, Inc.: Pittsburgh, PA, 1998.
22. Schmidt, M. W.; Baldridge, K. K.; Boatz, J. A.; Elbert, S. T.; Gordon, M.
S.; Jensen, J. H.; Koseki, S.; Matsunaga, N.; Nguyen, K. A.; Su, S.; Windus,
T. L.; Dupuis, M.; Montgomery, J. A. J. Comput. Chem. 1993, 14, 1347.![]()
23. Rittby, M.; Bartlett, R. J. J. Phys. Chem. 1988, 92, 3033.![]()
24. Knowles, P. J.; Hampel, C.; Werner, H.-J. J. Chem. Phys. 1994, 99, 5219.
25. Deegan, M. J. O.; Knowles, P. J. Chem. Phys. Lett. 1994, 227, 321.![]()
26. Peterson, K. A.; Woon, D. E.; Dunning, T. H., Jr. J. Chem. Phys. 1994,
100, 7410.![]()
27. Peterson, K. A.; Dunning, T. H., Jr. Private communication.
28. Davidson, E. R.; Ishikawa, Y.; Malli, G. L. Chem. Phys. Lett. 1981, 84,
226.![]()
29. Douglas, A. E.; Jones, W. J. Can. J. Phys. 1965, 43, 2216.![]()
30. Chase, M. W., Jr. NIST-JANAF Tables, 4th ed. J. Phys. Chem. Ref. Data,
Mono. 9, 1998, Suppl. 1.![]()
31. Jenkins, H. D. B.; Roobottom, H. K.; Passmore, J.; Glasser, L. Inorg. Chem.
1999, 38, 3609.
Jenkins, H. D. B.; Tudela, D.; Glasser, L. Inorg. Chem.
2002, 41, 2364.![]()
32. Zhan, C.-G.; Dixon, D. A. J. Phys. Chem. A 2001, 105, 11534.
Zhan, C.-G.; Dixon, D. A. J. Phys. Chem. A 2002, 106, 9737.
Zhan, C.-G.; Chipman,
D. M. J. Chem. Phys. 1998, 109, 10543.![]()
33. Becke, A. D. J. Chem. Phys. 1993, 98, 5648.
Lee, C.; Yang, W.; Parr, R.
G. Phys. Rev. B 1988, 37, 785.
Stephens, P. J.; Devlin, F. J.; Chabalowski,
C. F.; Frisch, M. J. J. Phys. Chem. 1994, 98, 11623.![]()
34. Huber, K. P.; Herzberg, G. Molecular Spectra and Molecular Structure: Constants of Diatomic Molecules; Van Nostrand Reinhold Col, Inc.: New York, 1979; Vol. 4.
35. Brazier, C. R.; Bernath, F. P.; Burkholder, J. B.; Howard, C. J. J. Chem.
Phys. 1988, 89, 1762.![]()
36. Polak, M.; Gruebele, M.; Saykally, R. J. J. Am. Chem. Soc. 1987, 109,
2884.![]()
37. Fletcher, G. D.; Gordon, M. S.; Bell, R. S. Theor. Chem. Acc. 2002, 107,
57.![]()
38. Lein, M.; Frunzke, J.; Timoshkin, A.; Frenking, G. Chem.-Eur. J. 2001, 7,
4155.![]()
39. Jacox, M. E. J. Phys. Chem. Ref. Data 1994, Monograph No. 3.
40. Polak, M.; Gruebele, M.; Saykally, R. J. J. Chem. Phys. 1988, 89, 110.
41. Sherman, W. F.; Wilkinson, G. R. In Vibrational Spectroscopy of Trapped Species; Hallam, H. E., Ed.; Wiley: London, 1973.
42. See for a quoted value for
1: Botschwina, P. J. Chem. Phys. 1986, 85,
4591.![]()
43. Pellerite, M. J.; Jackson, R. L.; Brauman, J. I. J. Phys. Chem. 1981, 85,
1624.![]()
44. Illenberger, E.; Comita, P. B.; Brauman, J. I.; Fenzlaff, H. P.; Heni, M.;
Heinrich, N.; Koch, W.; Frenking, G. Ber. Bunsen-Ges. Phys. Chem. 1985,
89, 1026.
Jackson, R. L.; Pellerite, M. J.; Brauman, J. I. J. Am. Chem. Soc.
1981, 103, 1802.![]()
45. Johnston, H. S. Gas-Phase Reaction Rate Theory; Ronald Press: New York, 1966. Steinfeld, J. I.; Francisco, J. S.; Hase, W. L. Chemical Kinetics and Dynamics; Prentice-Hall: Englewood Cliffs, NJ, 1989.
46. Landolt, B. Crystal Structure Data for Inorganic Compounds; Springer-Verlag: Berlin, 1993.
47. Wagman, D. D.; Evans, W. H.; Parker, V. B.; Schumm, R. H.; Halow, I.;
Bailey, S. M.; Churney, K. L.; Nutall, R. L. J. Phys. Chem. Ref. Data
1982, 11, Supplement No. 2.
48. The energy of the N7 + N3 channel is 324 kcal/mol above 5N2 molecules using the G3 heat of formation of N7, and thus N7 + N3 is 27 kcal/mol above the N5+N5- ion pair.49 The barrier6 to form N7 + N3 from N5+/N5- is very similar to the endothermicity of the reaction, and this process again involves two open shell molecules. A closed shell asymptote of geometry similar to that of the end-on addition of N5+ to N5- is N8 + N2, which is 230 kcal/mol above 5N2 at the CCSD(T)/6-311G*//MP2/6-31G* level50 and, thus, substantially downhill from the ion pair by ~67 kcal/mol. The N8 molecule that is formed, azidopentazole, has a barrier to formation of 4 N2 of only 13-14 kcal/mol at the CCSD(T)/6-311G* level49 and 19 kcal/mol at the CASPT2/ANO-4s3p2d1f level.51
49. Wang, X.; Tian, A.; Wong, N. B.; Law, H.-K.; Li, W.-K. Chem. Phys.
Lett. 2001, 338, 367.![]()
50. Chung, G.; Schmidt, M. W.; Gordon, M. S. J. Phys. Chem. A 2000, 104,
5647.![]()
51. Gagliardi, L.; Evangelisti, S.; Bernhardsson, A.; Lindh, R.; Roos, B. O.
Int. J. Quantum Chem. 2000, 77, 311.![]()
52. Nature, Science Update, May 15, 2002. Scientific American, News, May 15, 2002. Die Welt, May 15, 2002.
53. Schmidt, E. W. Hydrazine and its Derivatives Preparation, Properties, Applications; John Wiley & Sons: New York, 1984.
|
species |
basis |
r (NN) |
|
|
N2( |
CCSD(T)/aug-cc-pVDZ |
1.1209 |
|
|
|
CCSD(T)/aug-cc-pVTZ |
1.1040 |
|
|
|
CCSD(T)/aug-cc-pVQZ |
1.1005 |
|
|
|
CCSD(T)/aug-cc-pV5Z |
1.0995b |
|
|
|
expt34 |
1.0977 |
|
|
N3( |
CCSD(T)/aug-cc-pVDZ |
1.1997 |
180.0c |
|
|
CCSD(T)/aug-cc-pVTZ |
1.1840 |
|
|
|
CCSD(T)/aug-cc-pVQZ |
1.1802 |
|
|
|
expt35 |
1.18115 |
|
|
N3-( |
CCSD(T)/aug-cc-pVDZ |
1.2072 |
180.0c |
|
|
CCSD(T)/aug-cc-pVTZ |
1.1912 |
|
|
|
CCSD(T)/aug-cc-pVQZ |
1.1876 |
|
|
|
expt36 |
1.1884 |
|
|
N5-( |
CCSD(T)/aug-cc-pVDZ |
1.3429 |
108.0c |
|
|
CCSD(T)/aug-cc-pVTZ |
1.3309 |
|
|
N5+( |
CCSD(T)/aug-cc-pVDZ |
1.1319 |
165.87 |
|
|
|
1.3413 |
107.90 |
|
|
CCSD(T)/aug-cc-pVTZ |
1.1159 |
167.08 |
|
|
|
1.3238 |
108.48 |
|
|
expt2 |
1.10 |
168.1 |
|
|
|
1.30 |
111.2 |
|
N5(2A1)d |
ZAPT2/6-311+G(2df) |
1.292 |
121.0 |
|
|
|
1.343 |
100.1 |
|
|
|
1.355 |
109.5 |
|
|
CCSD(T)/aug-cc-pVDZ |
1.422 |
102.3 |
|
|
|
1.165 |
137.7 |
|
|
|
2.576 |
81.1 |
|
N5--TSe |
MP2/aug-cc-pVDZ |
1.270 |
125.5 |
|
|
|
1.702 |
99.4 |
|
|
|
1.215 |
107.8 |
|
|
CCSD(T)/6-311+G(d)7 |
1.252 |
128.9 |
|
|
|
1.764 |
|
|
|
|
1.191 |
|
a Bond distances in angstroms and bond angles in degrees.b Core/valence
correlation at the CCSD(T)/cc-pCVQZ level shortens the bond length by
0.0020 Å, resulting in an estimated CCSD(T)/aug-cc-pV5Z+CV value of
1.0975 Å.c Constrained by symmetry to these angles. Linear for N3 and
N3- and D5h for N5-.d The radical is cyclic with the symmetry unique
atom N1 at the apex. N1 is bonded to N2 and N5, and N2 is bonded to N3,
and N3 is bonded to N4. The bond distances are in the order: r(N1-N2)
and r(N1-N5); r(N2-N3) and r(N4-N5); and r(N3-N4). The bond angles
are in the order
N2N1N5;
N1N2N3 and
N1N5N4; and
N2N3N4
and
N5N4N3.e The transition state for the anion decomposition is cyclic
with the symmetry unique atom N1 at the apex. N1 is bonded to N2 and
N5, and N2 is bonded to N3, and N3 is bonded to N4. The bond distances
are in the order r(N1-N2) and r(N1-N5); r(N2-N3) and r(N4-N5); and
r(N3-N4). The bond angles are in the order
N2N1N5;
N1N2N3 and
N1N5N4; and
N2N3N4 and
N5N4N3.
|
method |
mode number |
mode symmetry |
mode description |
|
expt |
|
N2 |
|||||
|
CCSD(T)/aug-cc-pVDZ |
1 |
|
N2 str |
2319 |
2331a (2358.6) |
|
CCSD(T)/aug-cc-pVTZ |
1 |
|
N2 str |
2340 |
|
|
CCSD(T)/aug-cc-pVQZ |
1 |
|
N2 str |
2354 |
|
|
CCSD(T)/aug-cc-pV5Z |
1 |
|
N2 str |
2359b |
|
|
N3 |
|||||
|
MP2/cc-pVTZ |
1 |
|
bendh |
594 |
457c |
|
|
2 |
|
symmetric str |
1434 |
1320c |
|
|
3 |
|
asymmetric str |
1620 |
1645c |
|
N3- |
|||||
|
CCSD(T)/aug-cc-pVDZ |
1 |
|
bend |
578 |
626d |
|
|
2 |
|
symmetric str |
1281 |
1335e |
|
|
3 |
|
asymmetric str |
1999 |
1986f |
|
N5- |
|||||
|
CCSD(T)/aug-cc-pVDZ |
1 |
e1' |
NN str |
1202 |
|
|
|
2 |
a1' |
NN str |
1141 |
|
|
|
3 |
e2' |
NN str |
1078 |
|
|
|
4 |
e2' |
bend |
1001 |
|
|
|
5 |
e2' ' |
bend |
739 |
|
|
MP2/aug-cc-pVDZ |
1 |
e1' |
NN str |
1143 |
|
|
|
2 |
e2' |
NN str |
1123 |
|
|
|
3 |
a1' |
NN str |
1094 |
|
|
|
4 |
e2' |
bend |
1039 |
|
|
|
5 |
e2' ' |
bend |
740 |
|
|
N5+ |
|||||
|
MP2/aug-cc-pVDZ |
1 |
b2 |
NN str |
2260 |
2267g |
|
|
2 |
a1 |
NN str |
2179 |
2206g |
|
|
3 |
b2 |
NN str |
1199 |
1064g |
|
|
4 |
a1 |
NN str |
881 |
870g |
|
|
5 |
a1 |
bend |
669 |
671g |
|
|
6 |
b2 |
bend |
431 |
414g |
|
|
7 |
a2 |
out-of-plane bend |
426 |
474g |
|
|
8 |
b1 |
bend |
374 |
421g |
|
|
9 |
a1 |
bend |
179 |
204g |
|
N5--TS |
|||||
|
MP2/aug-cc-pVDZ |
1 |
b2 |
NN str |
1649 |
|
|
|
2 |
a1 |
NN str |
1572 |
|
|
|
3 |
a1 |
NN str |
1244 |
|
|
|
4 |
a1 |
NN str |
905 |
|
|
|
5 |
b2 |
bend |
848 |
|
|
|
6 |
b1 |
bend |
684 |
|
|
|
7 |
a2 |
out-of-plane bend |
591 |
|
|
|
8 |
b2 |
bend |
182 |
|
|
|
9 |
a1 |
NN str |
862i |
|
|
N5 (cyclic) 2A1 |
|||||
|
ZAPT2/6-311+G(2df) |
1 |
b2 |
NN str |
1221 |
|
|
|
2 |
a1 |
NN str |
1147 |
|
|
|
3 |
a1 |
NN str |
1064 |
|
|
|
4 |
b2 |
NN str |
1033 |
|
|
|
5 |
a1 |
NN str |
1002 |
|
|
|
6 |
a1 |
bend |
843 |
|
|
|
7 |
b2 |
bend |
798 |
|
|
|
8 |
a2 |
out-of-plane bend |
729 |
|
|
|
9 |
b1 |
bend |
363 |
|
a Reference 34. Value in parentheses is the harmonic value.b Core/valence correlation at the CCSD(T)/cc-pCVQZ level of theory increases the harmonic frequency by 9.2 cm-1, resulting in an estimated CCSD(T)/aug-cc-pV5Z+CV value of 2368 cm-1.c Reference 39.d Lamoureux, R. T.; Dows, D. A. Spectrochim. Acta, Part A 1975, 31, 1945. From N3- in a KI lattice.e References 41 and 42.f Reference 36.g Reference 2.h Average of 565 and 622 cm-1.
|
contributiona |
N (4S) |
N2 (1 |
N3 (2 |
N3- (1 |
N5- (1A1') |
N5+ (1A1) |
N5-TS (1A1) MP2 |
N5-TS (1A1) ref 7 geom |
|
aug-cc-pVDZb |
-54.486849 |
-109.295320 |
-163.770896 |
-163.863661 |
-273.142269 |
-272.683885 |
-273.101846 |
-273.099657 |
|
aug-cc-pVTZb |
-54.516714 |
-109.380845 |
-163.900633 |
-163.997758 |
-273.360072 |
-272.900359 |
-273.317071 |
-273.315909 |
|
aug-cc-pVQZb |
-54.525300 |
-109.407243 |
-163.939895 |
-164.038815 |
-273.428772 |
-272.965446 |
-273.383465 |
-273.382442 |
|
Est. CBS eq 1c |
-54.530069 |
-109.422126 |
-163.961942 |
-164.061926 |
-273.467671 |
-273.001946 |
-273.420892 |
-273.419928 |
|
|
|
227.15 |
233.26 |
296.00 |
512.87 |
220.63 |
483.52 |
482.91 |
|
|
|
0.65 |
1.03 |
1.22 |
1.66 |
1.80 |
|
|
|
|
|
-0.11 |
-0.51 |
-0.51 |
-1.04 |
-0.85 |
|
|
|
|
|
-3.35 |
-5.54 |
-6.53 |
-13.12 |
-12.27 |
-10.96 |
-10.0 |
|
|
|
224.34 |
228.34k |
290.18 |
500.37 |
209.31 |
|
|
|
|