Trialkylaluminum Hydride Compounds
Organometallics, Vol. 21, No. 13, 2002 2753
Ta ble 1. Ca lcu la ted a n d Exp er im en ta l Ver tica l Ion iza tion En er gies (in eV) of th e Mon om er a n d Dim er of
a
Tr im eth yla lu m in u m (TMA)
calculated
statec
assignmentb
HF/Koopmans
OVGF
EOM-CCSD
experimental
Monomer (C3h)
E′
A′
σAl-C
σAl-C
σC-H
10.47
13.78
14.1-14.6
9.54
12.83
13.2-13.7
9.57
12.81
13.2-13.7
9.85
12.6
13.3-14.0
Dimer (C2v)
B2
A1
B1
A1
B2
σAl-C
10.49
10.51
11.08
11.22
12.05
14.1-16.3
9.39
9.44
9.94
10.09
10.96
13.1-15.0
9.42
9.46
9.98
9.75
σAl-C
σAl-µC-Al
σAl-C + σµC-µC
σAl-C
10.45
10.96
13.0-15.0
11.2
12.0-16.2
σC-H
a
The calculations have been performed for the HF/6-31G** optimized geometries, using the 6-31G** basis set for HF/Koopmans, OVGF,
and EOM calculations. Assignments are based on the population analysis of the HF orbitals. c Given for the lowest, experimentally
b
separable states only.
B. HeI P h otoelectr on Sp ectr oscop ic Mea su r em en ts.
atory calculations were performed using 6-31G**, cc-pVDZ,
and aug-cc-pVDZ basis sets and the HF/6-31G** and MP2/6-
31G** optimized structures. Since the maximum difference
between these results does not exceed 0.3 eV, calculations for
all other species were performed for the HF/6-31G** optimized
structures only. For the ionization energy calculations the
6-31G** basis set was used.
(As Supporting Information HOMO and LUMO energies,
which can be useful in order to estimate the gas phase Lewis-
acid character of the investigated compounds, are also pre-
sented.)
HeI photoelectron (PE) spectra were recorded on an ATOMKI
3
8
ESA-32 spectrometer using a pyrolizer inlet system heatable
up to 350 °C. The accuracy of the temperature measurement
is estimated to be (10 °C. The sample pressure at the
-
6
-5
ionization chamber was kept between 8 × 10 and 4 × 10
mbar in each experiment. The full width at half-maximum of
the P3/2 peak of argon was 20-50 meV during the measure-
2
ments of TMA and DMA and 50-100 meV in the case of TEA
and DEA. The maximum error in ionization energies is
estimated to be less than 0.05-0.1 eV. All spectra were
calibrated against argon or nitrogen as internal standards; the
background corrections were made by Shirley-type functions.
The spectra of the dimers have been obtained by subtracting
the spectra recorded at high temperatures from the low-
temperature ones.
Resu lts a n d Discu ssion
A. Tr im eth yla lu m in u m . Berthomieu et al.31 have
recently calculated the first vertical and adiabatic
ionization energy of the TMA monomer and dimer by
∆HF, ∆MP2, and ∆DFT methods. Despite the small
difference (<0.1 eV) between the first vertical ionization
energies obtained by ∆HF and ∆MP2 methods, they
have concluded on the basis of ∆DFT calculations that
C. Ab In itio Ca lcu la tion s. Ab initio geometry optimiza-
3
9
tions were carried out by the PQS 2.1 program system. Outer-
4
0
valence Green’s function (OVGF) ionization energies have
4
1
been obtained by Gaussian98, while the ACESII program
4
2
package was used to compute ionization energies in the
framework of the equation of motion (EOM) CCSD method.43
Geometry optimizations have been performed for the ex-
“the [first] ionization energy of the dimer is lower than
4
,12
4,31
perimentally found
and theoretically confirmed
global
that of the monomer, by about 1 eV, which indicates
minimum structures (Figure 1) only. The optimizations were
followed by second derivative calculations to determine whether
the obtained stationary points correspond to minima. The
dependence of the calculated ionization energies on the
geometry and on the basis set was verified by OVGF calcula-
tions for the monomer and the dimer of TMA. These explor-
+
+
that TMA and TMA2 could be separated by ionization
techniques”. Our ionization energy calculations (Table
1
) do not support their conclusion, but they are in good
agreement with their ∆HF and ∆MP2 results. Although
the first ionization energy of the monomer and the dimer
might not be significantly different, our calculations also
predict regions in the photoelectron spectrum where the
dimer could be distinguished from the monomer unam-
biguously. These characteristic bands of the dimer are
expected to appear at about 10.0, 11.0, and above 14.0
eV, and they are separated from the closest bands of
the monomer by about 0.5, 1.5, and 0.5-0.9 eV, respec-
tively.
(
38) Cs a´ kv a´ ri, B.; Nagy, A.; Zanathy, L.; Szepes, L. Magyar K e´ miai
Foly o´ irat 1992, 98, 415.
39) PQS version 2.1; Parallel Quantum Solutions: Fayetteville, AR,
998.
40) (a) Cederbaum, L. S. Adv. Chem. Phys. 1977, 36, 205. (b) von
Niessen, W.; Schirmer, J .; Cederbaum, L. S. Comput. Phys. Rep. 1984,
, 57. (c) Oritz, J . V. J . Chem. Phys. 1988, 89, 6348. (d) Zakrzewski, V.
G.; von Niessen, W. J . Comput. Chem. 1993, 14, 13.
41) Frisch, M. J .; Trucks, G. W.; Schlegel, H. B.; Scuseria, G. E.;
(
1
(
1
(
Robb, M. A.; Cheeseman, J . R.; Zakrzewski, V. G.; Montgomery, J . A.,
J r.; 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.; Baboul, A. G.; 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.;
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Gordon, M.; Replogle, E. S.; Pople, J . A. Gaussian 98, Revision A.7;
Gaussian, Inc.: Pittsburgh, PA, 1998.
The experimental photoelectron spectra of TMA re-
corded at different temperatures are shown in Figure
2
. In the low-temperature spectra the above-mentioned
bands, characteristic for the dimer, can be observed at
only slightly higher ionization energies than predicted
by our calculations. Furthermore, the intensity of these
bands decreases rapidly with the increase of tempera-
ture, indicating the dissociation of the dimers. At about
75 °C the dissociation of the dimers is completed (i.e.,
the dimer bands are not recognizable in the spectrum,
which means that the dimer concentration is below a
few percent). Above this temperature, up to 200 °C, the
(
42) Stanton, J . F.; Gauss, J .; Watts, J . D.; Lauderdale, W. J .;
Bartlett, R. J . Int. J . Quantum Chem., Quantum Chem. Symp. 1992,
6, 897.
43) Stanton, J . F.; Bartlett, R. J . J . Chem. Phys. 1993, 98, 7029.
2
(