D. Zorrilla (Universidad de Cádiz, Spain)
J. Fernández Rico, R. López, G.
Ramrírez, I. Ema, F. Martínez
(Universidad Autónoma de Madrid, Spain)
S. Gadre (Savitribal Phule Pune U., India)
A. Kumar (University of Maryland, USA)
S. Yeole (Bushawal Arts, Science, and P.O. Nahata Commerce College, India)
Departamento de Química Física Aplicada, Facultad de
Ciencias C-XIV,
Universidad Autónoma de Madrid, 28049 Madrid, Spain.

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Introduction
Molecules can be regarded as sets of nuclei embedded in the negative
charge cloud generated by their electrons. The shape and size of this
cloud changes from one electronic state to another and, in a given
state, with the particular arrangement (conformation) of the nuclei.
However, not all states and nuclear conformations present the same
interest.
Considering the electronic states, it is specially relevant the ground
state in which most chemical processes occur. Among all the possible
nuclear arrangements in this state, the equilibrium conformation is
basic because, in the unperturbed stable molecule, nuclei usually tend
to remain around this position.
The features of the electron cloud are completely determined by the
electron density,
,which gives the probability per volume unit (density of probability) of
finding any electron at every point of space.
Electron density and its functionals are taking an increasingly central
role in the conceptual and practical development of the theoretical
chemistry. Indeed, this is due in part to the wide acceptation of the
density functional theory (DFT), but density has intrinsic merits to
occupy this place.
Electron density is an observable that can be experimentally measured
and which determines all the remaining local one-electron observables.
Though this is interesting because many of these observables play
relevant roles, even more important is the fact that density determines
all the chemical forces and hence the chemical behavior. This fact,
which sets the study of electron density as the central problem of
chemistry, deserves a short digression.
In the Born-Oppenheimer approximation (the paradigm in the study of the
molecular structure) the electronic energy is the potential energy for
the movement of the nuclei and, as a consequence, the components of the
force acting on a nucleus are the derivatives of the electron energy
with respect to the coordinates of that nucleus (multiplied by -1). The
Hellmann-Feynman (electrostatic) theorem states that these derivatives
are equal to the components of the electrostatic force generated by the
electron cloud plus the remaining nuclei. Thus, the forces can be
obtained in two ways: from the electronic energy and its derivatives or
from the electron density using classical electrostatics. The first way
is expensive and hardly provides chemical insight. The second one is
very cheap to apply and plenty of chemical insight.
Nonetheless, in spite of the fact that electrostatic theorem is known
more than sixty years ago, the possibilities that it opens have been not
exploited, and today the theorem is mostly regarded as a scientific
curiosity. There have been two main reasons for this. The first one is
that the fulfillment of the theorem requires high quality densities. In
particular, it leads to disastrous results for densities computed with
commonly used poor basis sets, whereas energy is less sensitive to the
quality of the basis set. The second reason comes from the fact that,
for extracting chemical information from the theorem, one needs a
representation of the density that brings insight to chemists.
These reasons no longer hold. As it has been reently proved, densities
computed with good Slater basis sets, and with very high quality
Gaussian basis sets too, fulfill the electrostatic theorem with an
accuracy that is sufficient for most quantitative applications and, a
fortiori, for the qualitative ones. Moreover, it has been also reported
a representation of the density aimed to retain the identity of the
atoms in a molecule as much as possible and that, in turn, facilitates
the application of the electrostatic theorem.
Basically, in this method the molecular density is partitioned into
minimally deformed pseudoatomic densities, which are achieved by
assigning to each atom the charge distributions centered on its nucleus
plus the part of the two-center ones closer to it. This partition
ensures that atomic densities exactly reproduce (on summation) the whole
density and, furthermore, that pseudoatomic densities can be accurately
represented in terms of rapidly convergent expansions in regular
harmonics times radial factors.
The method can be applied to densities calculated with Slater or
Gaussian basis sets and has been implemented in the DAM (Slater) and
G-DAM (Gaussian) programs.
This representation was originally intended as an aid for the
calculation of several functionals of the electron density such as the
molecular electrostatic potential, molecular force field, forces on
nuclei, etc, and it was proved to be very useful for this purpose. The
method was also applied to the analysis of binding forces and to the
calculation of bonding energies from the density in diatomics, as well
as to the explanation of the rotational barrier of ethane in terms of
the density.
These studies render evident that, combining this representation of the
density with the electrostatic theorem, basic concepts of chemistry can
be regarded from a novel perspective that may help to build a bridge
between electron density and the classical notions of the empirical
structural chemistry. The exploration of this possibility is the aim of
the content of this web page. Readers interested in how the deformed
atoms in molecules method describes the density and how the
electrostatic theorem can be combined with this description may get
further information by clicking here.
The formal developments of this method are detailed in the references
listed in the bibliography and its basic ideas are clarified herein with
an illustrative example.