Inelastic neutron scattering experiments are combined with infrared an
d Raman data to obtain a uniquely defined description of the intramole
cular vibrations of three oligomers of polythiophene, Through refineme
nt of ab initio force fields, the three vibrational spectra of each ol
igomer are simulated with remarkable accuracy. Two different basis set
s of atomic orbitals are used: the first, is 6-31G and is used to opt
imize the geometries,and calculate the relevant force fields of alpha-
2T and alpha-4T, the second is 3-21G and is used for the same purpose
for alpha-4T and alpha-6T. To improve agreement with the experiment,
the force fields are scaled. In this way, one set of scaling parameter
s is generated for the 6-31G basis and another for the 3-21G* basis.
The parameters are common to both molecules calculated with either bas
is sets and are believed to be transferable to higher isomers, The fit
ting procedure is applied in steps: first, the calculated vibrational
frequencies are assigned on the basis of the experimental infrared and
Raman activity, then a fitting of the Inelastic Neutron Scattering pr
ofile is performed, finally, the infrared and Raman spectra are calcul
ated with the new normal modes and the ab initio derivatives of the di
pole moment and the polarizability. The procedure is iterated until th
e three spectra of each oligomer are satisfactorily reproduced. For al
pha-4T, two scaled force fields are obtained-one for each basis set-an
d are shown to yield very similar normal modes. It is important to emp
hasize that not only the vibrational frequencies but also the spectral
intensities are well reproduced by the simulations. Implicitly, this
means that the dipole moment and the polarization tensor surfaces calc
ulated nb initio at the potential energy surface minimum are of good q
uality. The procedure is absolutely general and can be applied to any
molecular system. In the present case, it leads to well defined force
fields that give us a stringent picture of the vibrations of these mol
ecules. (C) 1996 American Institute of Physics.