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Coupling of angular momenta: electronic states
247
total orbital angular momentum is the orbital angular momentum of that sole electron, and
we can identify a corresponding one-electron orbital angular momentum quantum num-
ber λ = 0, 1, 2, 3, etc., which corresponds to σ, π, δ, and φ orbitals, respectively (see
Section 4.2.2). Note that the orbitals with non-zero λ are doubly degenerate, which may
be viewed as being due to the two possible directions for rotation of the electrons around
the internuclear axis, clockwise or anticlockwise. In this sense the projection of orbital
angular momentum on the internuclear axis is a signed quantity, but the convention is that
λ is always quoted as a positive number. The reader should recognize however that if,
for example, λ = 1 then the actual orbital angular momentum along the internuclear axis
is +
h or −h.
If there is more than one electron, each electron will contribute ±λ
h to the orbital
angular momentum along the internuclear axis. All filled orbitals will therefore make a
zero contribution to since the orbital angular momenta of the electrons in these orbitals
cancel. If there are two unpaired electrons, say one in a π orbital and one in a δ orbital, the
possible angular momenta are ±
h, ±2 h, or ±3 h. These correspond to = 1, 2, or 3 and
the resulting electronic states are labelled as , , and electronic states, respectively. A
better and more general way of deriving the possible orbital angular momentum states is
by recognizing that the σ, π, δ, etc., labels are actually symmetry labels for the molecular
orbitals, i.e. they are irreducible representations of the appropriate linear molecule point
group, D
∞h
or C
∞v
. The overall angular momentum must therefore also correspond to one
of the irreducible representations of the point group and can be obtained by taking the
direct product of the symmetries for each occupied orbital, and taking appropriate care in
the application of the Pauli principle (see below). This was the recommended procedure
covered in Part I.
The axial electric field in linear molecules does not have a direct effect on the spin angular
momenta, since spin is a magnetic phenomenon. However, when = 0 the orbiting motion
of the electron(s) generates a magnetic field,
1
which can also cause the total spin angular
momentum, S,toprecess around the internuclear axis. This is none other than spin–orbit
coupling, but if the spin–orbit coupling is not as strong as the spin–spin coupling then S
remains a good quantum number. As in the case of orbital angular momenta, the projection
of S onto the internuclear axis is quantized. The projection quantum number is given the
symbol ,which is unfortunately the same as the label used to designate electronic states
with = 0. The allowed values of are −S, −S + 1,...,+S,where S may be integer or
half integer depending on the number of unpaired electrons.
As in the case of atoms, spin–orbit coupling leads to spin–orbit sub-states with different
energies. In this case the total electronic (orbital + spin) angular momentum is given by
the quantum number (= + ). Although is, like , ostensibly a signed quantum
number, the accepted convention is to quote the positive value, i.e. =| + |. The
complete label for electronic states in linear molecules is then
2S+1
.
As an example, consider the case of two electrons in two different π molecular orbitals
(the choice of different π orbitals avoids difficulties with the Pauli exclusion principle – see
1
Current flowing in a circular conductor generates a magnetic field perpendicular to the plane of the conductor.
We can use the same analogy for an orbiting electron around the internuclear axis to explain how it generates a
magnetic field due to its orbital motion.