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The magnitude of the ligand field splitting parameter in the
octahedral field can be determined from the frequency of maximum
absorption in the optical absorption spectrum.
This absorption arises from an electronic
transition from the t2g level to the eg
level. This is the most important form of electronic transition
in the transition metal complexes, but others are also observed,
and these transitions are generally observed in the visible and
ultraviolet regions.
The types of interactions are:
Ligand Spectra: Some ligands,
such as water and organic molecules, possess characteristic
absorption bands, normally in the UV range. These bands are
observed in the optical spectra of the complexes, but are somewhat
shifted in frequency.
Counter-Ion Spectra: When
there is an ionic complex in solution, it must have a counter
ion. The spectrum of the counter ion must be known in order
to fully interpret the spectrum due to the complex ion.
Charge Transfer Spectra:
These spectra arise from electronic transitions between orbitals
which are principally those of the metal in character and orbitals
which are largely those of the ligands in character.
Ligand Field Spectra: These
account for the transition observed above, and arise from transitions
between d-orbitals of the metal which have been split due to
the ligand field.
Charge Transfer Spectra
Some transition metal complexes have very intense
colours, such as the chromate (CrO42-) and
permanganate (MnO4-) ions, and these colours
arise from charge transfer transitions between orbitals of which
one is mainly a metal orbital and one is mainly a ligand orbital.
These transitions correspond to metal
oxidation, when an electron is transferred from the metal
to the ligand, or metal reduction,
when an electron is transferred from the ligand to the metal.
Ligand to Metal charge transfer:
This corresponds to metal reduction, so a metal which is easily
reduced and a ligand which is easily oxidized will result in
a low energy transition. Therefore, oxidizable anions like I-
often form complexes where the charge transfer absorption is
in the visible region, eg. TiI4 is violet, HgI2
is red, and AgI is yellow. The trend in frequency of absorption
of a range of similar complexes can be explained in terms of
the ease of oxidation of the ligand, eg. TiCl62-
has a higher absoprtion frequency than TiBr62-
because the Br- ligand is more easily oxidized than
the Cl- ligand. Similar trends are observed when
the metal cation is strongly oxidizing, where the frequency
of absorption follows the oxidizing strength of the metal ion.
Metal to Ligand charge transfer:
This corresponds to metal oxidation, so it is necessary for
the metal to be easily oxidizable and the ligand to be easily
reducible. Easily reducible ligands are those which have a low
lying, vacant π* orbital, such as
pyridene, and they form strongly coloured complexes with easily
oxidizable metal cations such as Fe2+ and Cu+.
Depending of the d-number of the cation, two different transitions
are possible; the t2g to π*
and eg to π* may both
be observed.
Metal to Metal charge transfer:
Some compounds possess metal ions in two different oxidation
states. In these compounds, a charge transfer transition may
occur when the electron moves from one metal ion to the other,
with one metal ion acting as the reducing agent and the other
acting as the oxidizing agent. Compounds of this nature are
generally very intensely coloured, such as Prussian
Blue, KFeIII[FeII(CN)6].
These charge transfer transitions give intense absorptions
in the UV, but which trail into the visible region. Their intensity
means that they are strongly coloured, and so often obscure
the ligand field spectra.
Ligand Field Spectra
When an electron moves from one d-orbital to another,
as in the case of the t2g-to-eg transition,
the overall energy of the transition needs to take into account
the rearrangement of the other electrons when the transition occurs.
The possible transitions which may occur are governed by the possible
arrangements of electrons within the d-orbitals before and after
the transition takes place.
The possible transitions may be summarized in terms
of the selection rules, which come
from considering the effects of the coupling
of spin and orbital angular momentum in the ion, and the way this
changes during the transition on absorption of a photon. The cations
of the first row transition metals undergo Russell-Sauders
coupling.
Russell
Saunders coupling: the d2 ion |
When more than one valence electron
is present, interactions between the electrons result in
couplings between the quantum numbers for the individual
electrons. The quantum state of the overall ion depends
on the quantum states of the individual electrons.
The quantum state of the electron is determined by the
values of n (the principal quantum number), l (the orbital
angular momentum quantum number), ml (the magnetic
quantum number), and s (the spin quantum number).
There may be coupling between the spin angular momenta
of two electrons, spin-spin
coupling, the orbital angular momenta of two electrons,
orbit-orbit coupling, and
the spin and orbital angular momenta of the same electron,
spin-orbit coupling.
In the Russell-Saunders scheme, the case for the first
row transition elements, and in general for elements up
to atomic number 30, the magnitude of coupling is assumed
to be in the order: |
| spin-spin
coupling > orbit-orbit coupling > spin-orbit coupling |
Spin-spin coupling:
The spin quantum number, S, for a system of electrons
is calculated from the spin quantum numbers, s1
and s2, for the separate electrons according
to

|
for the
d2 system,

|
Orbit-orbit coupling:
For two electrons with
orbital angular momentum quantum numbers l1
and l2, the total orbital angular momentum
quantum number, L, is
This is known as the Clebsh-Gordan
Series.
|
for the
d2 system,
l1 = l2 =2, so

|
Different values of L are referred to by different
term letters: S (L=0), P (L=1),
D (L=2), F (L=3), G (L=4), H (L=5), ... |
the d2
system has G, F, D, P, and S states |
Spin-orbit coupling:
The total angular momentum quantum number, J, is obtained
by coupling the total spin and orbital angular momenta according
to:
|
Different values of S can have
different numbers of values of J, or different numbers of
levels. The number of levels
possible for a given S number is the multiplicity,
given by (2S + 1). |
the d2 system
has multiplicity values
S = 1: (2S+1) = 3 (a triplet)
S = 0: (2S+1) = 1 (a singlet) |
The information on the possible values of S,
L and J as summarized in the term symbol:

Not all terms are allowed, as some would require electrons
with the same spin to occupy the same orbital, in contravention
of the Pauli exclusion principle. |
the d2
system has the possible terms:
3P, 3F, 1S,
1D, 1G |
| The relative order of the energies of these
terms is given by Hund's rules:
1) The most stable state is the one with the maximum
multiplicity
2) For a group of terms with the same multiplicity,
the one with the largest value of L lies lowest in energy. |
the ground
state term for the d2 system is:
3F |
The selection rules may be summarised:
Spin forbidden transitions:
Transitions in which there is a change in the number of unpaired
electron spins are forbidden, ie. for a transition to give optical
absorption ΔS
= 0. Transitions where ΔS
is non-zero are spin forbidden.
Orbitally forbidden transitions:
Transitions involving the redistribution of electrons within
a single quantum shell are forbidden. Thus d-to-d and p-to-p
transitions are forbidden but s-to-p and p-to-d transitions
are allowed, and correspond to transitions where
ΔL = +1 or -1. Transitions
of the type g-to-g and u-to-u are said to be parity
forbidden.
The fact that these selection rules are not strictly
obeyed allows us to see the colours of transition metals and
to observe ligand field spectra arising from d-to-d transitions.
The selection rules are broken in the following ways:
The spin forbidden rule is relaxed by spin-orbit
coupling. The intensities of spin forbidden bands increase
with the spin-orbit coupling constant. Spin forbidden bands
are, however, extremely weak
The orbital forbidden rule is relaxed by vibronic
coupling. A vibrational mode of the complex that is antisymmetric,
or of u parity, with respect to the center of symmetry of the
complex can mix with the electronic wavefunction. On mixing,
the ground state can become mixed with a g-type vibration and
the excited state may mix with a u-type vibration, and so a
g-to-g transition will acquire some g-to-u character and so
become weakly allowed.
Intensity stealing:
when a ligand-field transition occurs close to a charge transfer
band, mixing of the electronic wavefunctions of the forbidden
excited term and the allowed charge transfer level means that
electronic transitions to the excited term become allowed.
The intensities of absorption bands are measured
experimentally in terms of the molar absorption
coefficient (ε). When light
shines on a sample, as in a spectrophotometer, the optical
density, d, is measured, and this can be converted into
the molar absorption coefficient.
 |
I0 is the intensity of
light incident on the sample, and I is the intensity
of the emergent light. |
 |
c is the solution concentration,
in gmoldm-3, and l is the path length
of the light through the sample, in cm. |
Some typical molar absorption coefficients, and
the selection rules corresponding to the transition from which
they arise are given in the table:
| Type of transition |
Example |
Typical value of ε |
| Spin forbidden, Orbital forbidden |
[Mn(H2O)6]2+ |
0.1 |
| Spin allowed, Orbital forbidden |
[Ti(H2O)6]3+ |
10 |
| Spin allowed, Orbital partially
allowed by d-p mixing |
[CoCl4]2- |
5 x 102 |
| Spin allowed, Orbital allowed (charge
transfer) |
[TiCl6]2- |
104 |
The values of ε therefore
arise from the nature of the transition, in terms of how allowed
it is, and account, for example, for the pale pink colour of
the aqueous [Mn(H2O)6]2+ ion,
and the dark purple colour of the aqueous MnO4-
ion, which are familiar from titrations using permanganate as
the indicator.
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