The general set of f orbitals is used for non-cubic symmetry. Three of these orbitals are common with the cubic set.
The cubic set of orbitals is used in a cubic environment e.g., octahedral or tetrahedral.
Although being 'valence' electrons, the 4f electrons are essentially buried and screened from the chemical environment. The orbitals have high angular nodality - diffuse orbitals with a large number of angular nodes.
Most of bonding is ionic in character. The lanthanoids have a large metallic/cationic radius.
Coordination are typically large, being 7,8 and 9
6 is possible but requires bulky ligands
10 is possible but requires chelating ligands with a small bite angle
The lanthanoid contraction:
4f orbitals are not the outermost orbitals
3+ configuration has 5s and 5p electrons as size determining
Overlap between the probability function of 4f with 5s and 5p = poor at shielding
This gives a contraction of size
The average radialvelocity of an electron is proportional to atomic number, i.e. for heavier atoms there are relativistic effects on the mass of the electron. These effects account for ~ 10% of the lanthanoid contraction.
As a consequence of the large value of the 4th ionisation energy, 3+ predominates.
Ce, Pr and Tb are found in 4+ OS due to electron configurations
4f orbitals are at higher energy at the start of the series, therefore less energy required to remove 4th electron
Nd, Sm, Eu, Tm, Dy and Yb are found in 2+ OS with relatively increased 3rd ionisation energies
UV-Vis spectroscopy probes the transitions of valence electrons, including f-f transitions (forbidden).
d orbitals are influences by ligand field splitting
f orbitals have no ligand field effects
f orbitals are buried and sufficiently large to take into account the interaction between S and L (spin-orbit coupling)
The electronic spectra of Ln have many transitions, a large number of excited state terms.
Weak transitions, reduced vibronic coupling due to poor interaction with ligands
Sharp transitions, d-d transitions are broad as a consequence of different vibrational energy levels
Ln3+ does not interact with the ligand environment - colours are often indicative of the lanthanide.
4f - 5d transitions are allowed
Intense transitions at high energy
For Eu2+ energy of 4f is raised and transitions are in the visible region
For a general configuration of fn:
Microstates = 14!/n!(14-n)!
For each distinct combination of n electrons, there are n! permutations. For 2 different electrons:
When including J into the calculated number of microstates it creates a significant number of energy levels. The increased number of excited state terms means we can expect to see more f-f transitions.
Electronic excitation: an electron is promoted to an excited state (absorption spectroscopy).
Non-radiative decay: energy is lost as the excited state cascades to lower vibrational and rotation energy levels, a fast process.
Radiative decay: f electrons are not involved in bonding (vibration/rotation) and therefore f-f transitions are more likely to result in radiative decay (emission spectroscopy).
Direct excitation of the Ln series gives a small separation between the energy of the incoming photon and emitted photon - this is a Stokes shift.
The antenna effect is seen when Ln is excited indirectly using a ligand antenna, seen with aromatic ligands.
Fluorescence:
Short-lived
On the ps to ns timescale
Decay from an excited state of the same multiplicity to the ground state
Phosphorescence:
Long-lived
On the ns to μs scale
Decay from an excited state of a different multiplicity compared to the ground state
During the antenna effect, the ligand captures light and is promoted to an excited singlet - radiative decay occurs. There is then intersystems crossing (ISC) to an excited triplet, then excited states of Ln, then luminescence.
Intersystem crossing: at a certain point the potential energy of singlet and triplet states intersect and transfer between the two states is possible.
Internal transfer: similar to intersystems crossing, but there is no change in spin multiplicity.
Lifetimes of excited states:
Triplet state has a longer lifetime
Return to the ground state requires a spin-forbidden electronic transition
Energy between a triplet and singlet state cannot be lost through non-radiative decay
During quenching, energy is lost to the vibrational modes of solvated groups e.g., water. This encapsulates Ln with a multidentate ligand to avoid water coordination.
The magnitude of the magnetic dipole moment, μz, generated by an electron, with spin angular momentum, S is given by:
μeff = -gμBS
g = proportionality factor, a dimensionless constant dependent on environment (2.0023 for a free electron)
μB = the Bohrmagneton, a constant for expressing the magnetic moment of an electron (9.274 X 10-24 J T-1)
For a multi-electron system:
μeff = -g[S(S + 1)]1/2μB
S = total spin quantum number
Where orbitals are degenerate and can be transformed into each other via rotation, electrons are able to move between orbitals.
This creates an associated magnetic moment
This can only occur for d block compounds when there is an open shell t2g configuration
Where this is not the case the magnetism from orbital angular momentum is said to be quenched
All orbitals are degenerate in a free ion d block element. For a d1 system with an electron in the dxy orbital, the d(x^2-y^2) is equivalent in energy. The transformation is a single rotation and creates a magnetic moment, providing the orbital angular moment component of paramagnetism. The same principle can be applied to f orbitals.
The magnetic moment will be linked with total electron spin (S), electron orbit angular momentum (L) and the total angular momentum (J), which arises due to spin-orbit coupling.
gS = proportionality factor of an electron ~ 2
gL= electron orbital proportionality factor = 1
gJ = Lande proportionality factor, which is linked to J
There are different values of J and these create multiple f-f transitions.
The value of J is linked to the observed magnetic moment
In most cases, the energy difference between the ground state and excited state is thermally inaccessible
i.e. only the ground state J value is observed in magnetism
Where this is not the case we have exception from the J moment determined values
For Sm3+ and Eu3+ the energy difference between the ground and lowest energy excited state terms are thermally accessible. This causes a Boltzmann population distribution. This gives a mixture of J states which all contribute to the magnetic moment and causes deviations based on their relative population.
Pitchblende: ore of uranium with an abundance of 2.3 ppm (higher than tin).
Thorite: treatment with potassium gives thorium with an abundance of 8.1 ppm (more than boron).
Thorium and uranium are the only naturally occurring actinoids - the rest are formed using particle colliders and during nuclear explosions.
Naturally occurring actinoids:
Protactinium has two naturally occurring isotopes which arise due to radioactive decay of uranium
Alpha decay is the loss of a helium nucleus
Beta decay is a neutron into a proton, electron and antineutrino
Every known isotope of An's are radioactive.
Only 232Th, 235U and 238U have long enough half-lives to have survived since the formation of the solar system
Stability depends on atomic mass and numbers of protons/neutrons
Even number of proton and neutrons > odd numbers of protons, even of neutrons . Odd numbers of protons and neutrons
For s and p orbitals, direct scalar relativistic effects cause them to contract. This manifests by adding shielding for valence electrons. For d and f orbitals, they are expanded by a process known as indirect relativistic orbital expansion.
Contracted s and p orbitals provide better shielding and the orbitals are expanded
Binding energy of 5f electron is ~50% of expected
Destabilisation of f orbitals allows electrons to be removed more easily
Oxidation states of actinoids:
The lower the potential, the lower the Gibbs energy, the more stable the state is
The gradient between points is the potential of the redox couple
Early actinoids behave like transition metals (5f up to Np are involved in bonding)
Late actinoids are typically 3+ with 5f contracting along the series
Actinoids require a new model of spin-orbit coupling: j-j coupling.
Looks at the individual coupling for l and s for each electron to give j
Previous model works well for lanthanoids
For actinoids the spin-orbit coupling is not large enough to completely ignore interelectronic repulsions