Theoretical study demonstrates UV–vis spectroscopy's role in elucidating plutonium speciation in saline environments, suggesting improved characterization of aqua–chloro complexes.
Plutonium speciation in high-salinity media remains difficult to characterize, yet it largely governs the geochemical fate of PuO22+ in marine environments. EXAFS and UV–vis measurements established that the evolution of specific spectral features correlates with the formation of successive aqua–chloro complexes. These signals represent a superposition of coexisting species in equilibrium, masking the individual contributions of each complex. In this work, we address this limitation with a combination of the nuclear ensemble approach (NEA) and high-level quantum-mechanical calculations, accounting for the relativistic Hamiltonian, spin–orbit coupling, and electron correlation, to isolate these overlapping contributions of the [PuO2(H2O)mCln]2–n series and clarify the observed plutonyl speciation. The sensitivity of our methodology is quantified by comparing Wigner sampling against classical molecular dynamics (MD) trajectories. The results establish UV–vis spectroscopy as a high-resolution probe of the equatorial ligand field and provide a molecular basis for Pu(VI) speciation in saline environments.
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Raposo-Hernández et al. (2026) studied this question.
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