J. Chem. Phys., Vol. 109, No. 20, 22 November 1998
Nicola ¨ı et al.
9073
VIII. CONCLUSION
Rotational tunneling of the methyl group is highly sen-
sitive to the rotational potential, but this is only a useful
probe when it can be correlated with structure. The Coulomb
energy in crystals of organic compounds is frequently invari-
ant with the rotational conformation of the methyl group so
that calculations which use very approximate methods to ob-
tain the Coulomb terms give reasonable results. However,
the most interesting systems are those in which the correla-
tion between one-dimensional rotational dynamics and struc-
ture fails, since this points to novel dynamics, coupling, etc.
In these circumstances, problems with Coulomb interactions
need to be eliminated, or at least identified, before embarking
on a time-consuming study involving additional degrees of
freedom and coupling.
FIG. 11. Inelastic neutron scattering spectrum of Li͑CH COO͒, 2D O mea-
3
2
sured on TFXA ͑dotted line͒ and calculated spectrum with ab initio method
line͒.
͑
We have shown that point charges obtained from ab ini-
tio methods provide a reasonable approximation and that the
best results are obtained when these are recalculated for each
step in the reorientation of the methyl group. The main prob-
Acetate modes not involving the methyl group are much
more sensitive to the crystalline environment, the CC mode
Ϫ1
being found between 924 and 964 cm , while the CO
Ϫ1
mode arises anywhere between 1408 and 1595 cm
.
lem is the computational expense of this method, particularly
for large models. Whereas previous calculations1
0–15
have
It has been shown that if intermolecular interactions are
weak, the vibrational frequencies and amplitudes calculated
by ab initio methods should compare well with the frequen-
cies and intensities measured by INS.38 We have recorded
the INS spectrum of several metal acetates at liquid-helium
temperature on the IN1 spectrometer: cobalt acetate tetrahy-
drate, nickel acetate tetrahydrate, zinc acetate dihydrate, and
sodium acetate trihydrate. The vibrations of the water mol-
ecules dominate these spectra, but nevertheless, we can dis-
used a bigger basis set for the ab initio calculations
(6-31G**), this work shows that a much reduced basis set,
which is imposed by the chemical composition of the sys-
tem, is adequate in this case, the advantage being the reduc-
tion of the computing time.
Density functional methods ͑DFT͒ provide an accurate
alternative, but these require the use of a fairly large cell to
eliminate the rotation of neighboring methyl groups. With
our presently available computing resources we have been
unable to obtain satisfactory results for methyl dynamics in
the metal acetates.
tinguish the rocking modes of the methyl group at around
Ϫ1
1
050 cm in all these spectra.
Although the resolution of the IN1 spectrometer does not
allow us to separate the two methyl rocking modes in the
INS spectra we have also been able to record the spectrum of
Li͑CH COO͒.2D O using the TFXA spectrometer which has
ACKNOWLEDGMENTS
3
2
We thank M. F. Lautie from the LASIR-CNRS ͑Thiais,
´
higher resolution. Because the water was deuterated for this
compound, this spectrum is dominated by the vibrational
modes of the methyl group, and the two rocking modes of
the methyl group can be discerned as a maximum at 1050
France͒ for providing deuterated samples of cobalt acetate.
We thank P. Smith from ILL for assistance with the crystal-
structure determination of cobalt acetate. We are also grate-
ful to M. Neumann and P. Schiebel for helpful discussions.
Ϫ1
Ϫ1
cm with a shoulder at about 1070 cm ͑Fig. 11͒.
We performed ab initio calculations of the isolated ac-
Ϫ
etate group CH COO with GAMESS-UK, using the
1
3
Springer Tracts in Modern Physics, edited by W. Press ͑Springer, Berlin,
6
-31G* basis set with a complete optimized molecular ge-
1981͒.
2
3
4
ometry followed by a calculation of the harmonic frequen-
cies. These calculations predict the frequency and the rela-
tive intensity of the rocking modes at about 1040 and 1100
D. Cavagnat and M. Pesquer, J. Chem. Phys. 90, 3289 ͑1986͒.
B. M. Rice and S. F. Trevino, J. Chem. Phys. 94, 1991 ͑1990͒.
A. M. Alsanoosi, A. J. Horsewill, and S. Clough, J. Phys.: Condens.
Matter 1, 643 ͑1989͒.
A. Heidemann, M. Prager, and M. Monkenbush, Z. Phys. B 76, 77 ͑1989͒.
M. Prager, W. I. F. David, and R. M. Ibberson, J. Chem. Phys. 95, 2473
Ϫ1
5
6
cm with reasonable accuracy, a global scaling factor of
0
.95 having been introduced to account for the usual overes-
͑
1991͒.
timation of the force constants by ab initio methods. We
have made no attempt to analyze the other parts of the vibra-
tional spectrum as this is not of interest to the present work.
This simple model clearly shows that, at least in the
acetates, the methyl rocking modes are almost purely in-
tramolecular, any intermolecular terms being insignificant at
the present level of accuracy. The picture which emerges is
the acetate group, in any of its crystalline environments, be-
ing held in place by the oxygen atoms, with the methyl group
seeing a rather smooth potential energy surface from its sur-
rounding atoms.
7
8
A. M. Alsanoosi and A. J. Horsewill, Chem. Phys. 160, 25 ͑1992͒.
J. Meinnel, M. Mani, M. Nusimovici, C. J. Carlile, B. Hennion, R. Carrier,
B. Wyncke, M. Sanquer, and F. Tonnard, Physica B 202, 293 ͑1994͒.
M. Neumann and G. J. Kearley, Chem. Phys. 215, 253 ͑1997͒.
M. R. Johnson, B. Frick, and H. P. Trommsdorff, Chem. Phys. Lett. 187,
9
0
1
258 ͑1996͒.
11
M. R. Johnson, M. Neumann, B. Nicola ¨ı , P. Smith, and G. J. Kearley, J.
Chem. Phys. 215, 345 ͑1997͒.
M. Neumann and M. R. Johnson, J. Chem. Phys. 107, 1725 ͑1997͒.
B. Nicola ¨ı , G. J. Kearley, O. Randl, F. Fillaux, and P. H. Trommsdorff,
Physica B 234–236, 76 ͑1997͒.
B. Nicola ¨ı , E. Kaiser, F. Fillaux, G. J. Kearley, A. Cousson, and W.
Paulus, Chem. Phys. 226, 1 ͑1998͒.
1
1
2
3
14
Downloaded 19 Jun 2013 to 129.10.107.106. This article is copyrighted as indicated in the abstract. Reuse of AIP content is subject to the terms at: http://jcp.aip.org/about/rights_and_permissions