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Symmetry in Chemistry
From Wikipedia, the free
encyclopedia

Electron atomic and molecular
orbitals
In
quantum
chemistry, the molecular
electronic
states,
i.e. the
eigenstates
of the
electronic
molecular Hamiltonian, are
expanded (see
configuration interaction
expansion and
basis)
into
linear
combinations
of anti-symmetrized products (Slater
determinants) of one-electron
functions. The spatial components of these one-electron
functions are called molecular orbitals (MO). When
one considers also their
spin
component, they are called molecular spin orbitals.
Most methods in
computational chemistry today
start by calculating the MOs of the system. A molecular orbital
describes the behavior of one electron in the electric field
generated by the nucleii and some average distribution of the
other electrons. In the case of two electrons occupying the same
orbital, the
Pauli
principle demands that they
have opposite spin.
Hand-waving discussion
For hand-waving (imprecise, but
qualitatively useful) discussion of the molecular structure, the
molecular orbitals can be obtained from the "Linear
combination of atomic orbitals molecular orbital method"
ansatz
(using eventually the concept of
hybridized
orbitals).
In this approach, the molecular orbitals
are expressed as
linear
combinations of
atomic
orbitals, as if each atom were
on its own.
The
linear
combination of atomic orbitals
approximation for molecular orbitals was introduced in
1929
by
Sir John
Lennard-Jones. His
ground-breaking paper showed how to derive the electronic
structure of the
fluorine
and
oxygen
molecules from quantum principles. This qualitative approach to
molecular orbital theory represents the dawn of modern quantum
chemistry.
Some properties:
The number of molecular orbitals
is equal to the number the atomic orbitals included in the
linear expansion,
If the molecule has some symmetry, the
degenerate atomic orbitals (with the same atomic energy) are
grouped in linear combinations (called
symmetry adapted atomic orbitals (SO))
which belong to the
representation of the
symmetry
group,
The number of molecular orbitals
belonging to one group representation is equal to the number of
symmetry adapted atomic orbitals belonging to this
representation,
Within a particular
representation, the symmetry
adapted atomic orbitals mix more if their atomic
energy level
are closer.
Examples
H2
As a simple example consider the
hydrogen
molecule, H2, with the two atoms labelled H' and H".
The lowest-energy atomic orbitals, 1s' and 1s", do not transform
according to the symmetries of the molecule. However, the
following symmetry adapted atomic orbitals do:
|
1s' - 1s" |
Antisymmetric
combination: negated by reflection, unchanged by other
operations |
|
1s' + 1s" |
Symmetric combination:
unchanged by all symmetry operations |
The symmetric combination (called a
bonding orbital) is lower in energy than the basis orbitals, and
the antisymmetric combination (called an
antibonding
orbital) is higher. Because the H2 molecule has two
electrons, they can both go in the bonding orbital, making the
system lower in energy (and hence more stable) than two free
hydrogen atoms. This is called a
covalent
bond.
H3
On the other hand, consider the
hypothetical linear molecule of H3 with the atoms
labelled H, H' (the central atom), H" and equal H-H' and H'-H"
distances. Then we would expect three linear combinations:
1s - 1s' + 1s" Symmetric Anti
Bonding (2 nodal surfaces perpendicular to the bonds)
1s - 1s" Antisymmetric Non
bonding (1 nodal surface along the axis of symmetry)
1s + 1s' + 1s" Symmetric Bonding
(0 nodal surface)
Two electrons occupy the
symmetric bonding bonding orbital and the third one occupy the
non bonding orbital.
Rare gases
Now let's move to larger atoms.
Considering a hypothetical molecule of He2, since the
basis set of atomic orbitals is the same as in the case of H2,
we find that both the bonding and antibonding orbitals are
filled, so there is no energy advantage to the pair. HeH would
have a slight energy advantage, but not as much as H2
+ 2 He, so the molecule exists only a short while. In general,
we find that atoms such as He that have completely full energy
shells rarely bond with other atoms. (In fact there is not a
single stable molecule containing He, Ne or Ar except
short-lived
Van der
Waals complexes.)
Inner shells
Inner shell orbitals should not be
included in the
LCAO
expansion. Molecular structure relies on the outermost (valence)
electrons of the atoms, which are usually of comparable energy.
Ionic bonds
When the energy difference between the
atomic orbitals of two atoms is quite large, one atom's orbitals
contribute almost entirely to the bonding orbitals, and the
other's almost entirely to the antibonding orbitals. Thus, the
situation is effectively that some electrons have been
transferred from one atom to the other. This is called a
(mostly)
ionic bond.
More quantitative approach
To obtain quantitative values for the
molecular
energy
levels, one needs to have
molecular orbitals which are such that the
configuration interaction (CI)
expansion converges fast towards the
full CI
limit. The most common method to obtain such functions is the
Hartree-Fock
method which expresses the molecular orbitals as
eigenfunctions of the
Fock
operator. One usually solves
this problem by expanding the molecular orbitals as linear
combinations of
gaussian
functions centered on the
atomic
nuclei (see
linear
combination of atomic orbitals
and
basis set
(chemistry)). The equation for
the coefficients of these
linear
combinations is a generalized
eigenvalue
equation known as the
Roothaan
equations which are in fact a
particular representation of the
Hartree-Fock
equation. |