![]() |
|
![]() |
![]() |
Molecular Electronic Structure |
|||||||||||||||
The many-particle, three-dimensional time-independent Schrödinger (equation (2.20)) can be adapted for molecular systems. In this case, the molecular Hamiltonian becomes:
i and j refer
to electrons (of which there are n), and A
and B refer to nuclei (of which there are
N). 3.1 The Born-Oppenheimer approximation Solving the time-independent Schrödinger equation for a molecular
system (equation (3.1)) quickly becomes very complex.
As an example, benzene includes 861 electron-electron distances alone.
Thus, to obtain the electronic Schrödinger equation, the nuclear kinetic energy terms are omitted:
…where the electronic Hamiltonian is given by equation (3.4):
The nuclear repulsion term in the electronic Schrödinger equation, VNN, is given by equation (3.5):
The energy U in (3.3) is the electronic
energy including nuclear repulsion. The term VNN
is a constant, in that the wavefunction does not depend on VNN,
but there is a different wavefunction for each value of VNN.
The electronic wavefunction is said to be parametrically dependent on
the nuclear coordinates; this is shown by the underlined nuclear coordinate,
R, in equation (3.2).
This is related to the electronic energy including nuclear repulsion simply by the sum of the nuclear repulsion term, VNN:
Therefore, the electronic energy for a particular configuration of nuclei can be found by solving equation (3.6), and then U can be found using (3.7) and (3.5), with knowledge of the assumed nuclear coordinates. The nuclear Hamiltonian is given by equation (3.8):
The first term in this equation is the kinetic energy of the nuclei; the second term is their potential energy, and is often referred to as the inter-atomic potential energy surface (PES). |
||||||||||||||||
« Previous | Next » | ||||||||||||||||
[9] M. Born and J.R. Oppenheimer, Ann. d. Physik, 84, 457, 1927 |
![]() ![]() Potential Energy Surfaces and Conical Intersections • June 2002 • Ian Grant |