We applied relativistic
multiconfigurational all-electron
ab initio
calculations
including the spin–orbit interaction
to calculate the 3d4f resonant inelastic X-ray scattering (RIXS) map
(3d
3/2
→ 5f
5/2
U M
4
absorption
edge and 4f
5/2
→ 3d
3/2
U M
β
emission) of uranyl (UO
2
2+
). The calculated data are in excellent agreement
with experimental results and allow a detailed understanding of the
observed features and an unambiguous assignment of all involved intermediate
and final states. The energies corresponding to the maxima of the
resonant emission and the non-resonant (normal) emission were determined
with high accuracy, and the corresponding X-ray absorption near edge
structure spectra extracted at these two positions were simulated
and agree well with the measured data. With the high quality of our
theoretical data, we show that the cause of the splitting of the three
main peaks in emission is due to the fine structure splitting of the
4f orbitals induced through the trans di-oxo bonds in uranyl and that
we are able to obtain direct information about the energy differences
between the 5f and 4f orbitals: Δ5f δ/ϕ –
4f δ/ϕ, Δ5f π* – 4f π, and Δ5f
σ* – 4f σ from the 3d4f RIXS map. RIXS maps contain
a wealth of information, and
ab initio
calculations
facilitate an understanding of their complex structure in a clear
and transparent way. With these calculations, we show that the multiconfigurational
protocol, which is nowadays applied as a standard tool to study the
X-ray spectra of transition metal complexes, can be extended to the
calculation of RIXS maps of systems containing actinides.