Denecke, M. A.

Göttlicher, J.

Jorissen, K.

Kas, J. J.

Kvashnina, K.

Prüßmann, T.

Rehr, J. J.

Rothe, J.

Vitova, T.

English

KITopen

Journal of Physics: Conference SeriesOPEN ACCESSActinide and lanthanide speciation with high-energy resolution X-ray techniquesTo cite this article: T Vitova et al 2013 J. Phys.: Conf. Ser. 430 012117 View the article online for updates and enhancements.You may also likeResponse of HR-GaAs:Cr sensors tosubnanosecond X- and -ray pulsesI. Chsherbakov, P. Chsherbakov, A.Lozinskaya et al.-Selective Epitaxial Si:P Film for nMOSFETApplication: High PhosphorousConcentration and High Tensile StrainXuebin Li, Abhishek Dube, Zhiyuan Ye etal.-Magnetic ferrous-doped graphene forimproving Cr(VI) removalTing Hou, Lingyu Kong, Xiaoyu Guo et al.-This content was downloaded from IP address 141.52.109.171 on 28/04/2022 at 15:30      Actinide and lanthanide speciation with high-energy resolution X-ray techniques T Vitova1, M A Denecke1, J Göttlicher2, K Jorissen3, J J Kas3, K Kvashnina4, T Prüßmann1, J J Rehr3 and J Rothe1  1Karlsruhe Institute of Technology, Institute for Nuclear Waste Disposal, P.O. Box 3640, D-76021 Karlsruhe, Germany 2Karlsruhe Institute of Technology, Institute for Synchrotron Radiation, P.O. Box 3640, D-76021 Karlsruhe, Germany 3Department of Physics, University of Washington, Seattle, WA 98195, USA 4European Synchrotron Radiation Facility (ESRF), 6 Rue Jules Horowitz, BP 220, 38043 Grenoble Cedex 9, France   E-mail: Tonya.Vitova@kit.edu  Abstract. High-energy resolution X-ray absorption spectroscopy (HR-XAS) and Resonant inelastic X-ray scattering (RIXS) combined with quantum theoretical tools are gaining importance for understanding electronic and coordination structures of actinide (An) and lanthanide (Ln) materials. HR-XAS is successfully used to remove lifetime broadening by registering the partial fluorescence yield emitted by the sample, thereby yielding highly resolved X-ray absorption near edge structure spectra (HR-XANES), which often display resonant features not observed in conventional XANES. We demonstrate the structural characterization capabilities of these novel techniques by comparative discussion of U M4/L3-HR-XANES and L3-valence band RIXS (L3-VB-RIXS) spectra of two model U(VI) minerals.  We show that the ab initio multiple scattering theory based code FEFF9.5 is an effective tool for calculations of An and Ln L3-HR-XANES and L3-RIXS spectra as it successfully reproduces dipole and quadrupole transitions in the same spectrum. 1. Introduction High-energy resolution X-ray absorption near edge structure spectroscopy (HR-XANES) at the actinide (An), lanthanide (Ln) L3 edge and An M4,5 as well as An/Ln L3 valence-band and core-to-core resonant inelastic X-ray scattering (VB-RIXS, CC-RIXS) are currently developing techniques providing new insights into the An and Ln electronic structure [1,2]. The highly efficient X-ray emission spectrometers developed in the last years minimise the experimental spectral broadening to values significantly smaller than the core-hole lifetime broadening and thereby approach the energy resolution limit for HR-XANES spectra [3]. These instruments are based mostly on an array of bent analyser crystals in a Rowland circle geometry diffracting and focusing the fluorescence onto a detector and, for example, resolve pre-edge structures in Ln and U L3 edge HR-XANES (L3-HR-XANES) spectra [1,2]. Only few HR-XANES for U materials have been reported so far and the U pre-edge is clearly visible in U(VI) spectra [1]. This spectral resonance is interpreted as resulting from 2p3/2→5f electronic transitions, as corroborated by calculations with the FDMNES code. However, the calculated energy difference between the pre-edge and most intense resonance (white line, WL) is 15th International Conference on X-ray Absorption Fine Structure (XAFS15) IOP PublishingJournal of Physics: Conference Series 430 (2013) 012117 doi:10.1088/1742-6596/430/1/012117Published under licence by IOP Publishing Ltd 1      smaller (4.5 eV) than the experimental one (7 eV) [1]. We present calculations with the ab initio FEFF9.5 code [4], which agree well with the experimental spectrum. Additionally, we demonstrate that FEFF9.5 is able to calculate the pre-edge (2p3/2→4f/5f) and the WL (2p3/2→5d/6d) in both the An/Ln L3-HR-XANES and Ln L3-CC-RIXS spectra, whereas other theoretical approaches calculate these absorption resonances separately [2]. The capability of the HR-XANES technique to measure the relative energy difference between An/Ln f and d states in a system of materials with small structural variations is extremely valuable for tuning theoretical approaches. It will also shed light onto the degree of stabilisation of the An 5f valence orbitals across the actinide series and onto the amount of mixing in molecular orbitals between An/Ln valence with ligand orbitals. We also compare and discuss the sensitivity of the U L3/M4-HR-XANES and L3-VB-RIXS to geometric structural changes for the same U(VI) oxidation state.  2. Experimental part and calculation details The U L3/M4-HR-XANES, L3-VB-RIXS of Ca(UO2)2(PO4)2⋅10-12(H2O) (meta-autunite), NaCa3(UO2)(CO3)3(SO4)F⋅10(H2O) (schroeckingerite) and Yb L3-HR-XANES, L3-CC-RIXS of Yb2O3 were recorded at the ID26 beamline, ESRF, Grenoble [3]. The synchrotron radiation was monochromatized by a Si(311) (U L3 17166 eV, Yb L3 8944 eV)/Si(111) (U M4 3728 eV) double crystal monochromator (DCM). The experimental energy resolution was about 1.8 eV (U L3), 0.8 eV ( U M4) or 1.2 eV (Yb L3), measured as the width of the quasi-elastic peak. For each excitation energy, the emitted photons from the sample were diffracted by spherically bent Ge(777) (U Lα1 13614 eV), Si(220) (U Mβ 3339.8 eV) or Si(620) (Yb Lα1 7416 eV) analyzer crystals and focused onto a X-ray silicon drift detector (SDD KETEK). The sample, crystal and detector were positioned in Rowland circle geometry with 1m diameter, equal to the bending radius of the crystals. The conventional fluorescence mode U M4-XANES of (UO2)8O2(OH)12⋅12H2O (schoepite) was recorded at the INE-Beamline, ANKA, Karlsruhe [5] using a pair of Si(111) crystals in the DCM and detecting U Mß fluorescence with a photo diode. The U/Yb L3-HR-XANES and Yb L3-CC-RIXS calculations were performed with the ab initio multiple-scattering (MS) theory based FEFF9.5 code [4]. The atomic potentials were calculated self consistently on a cluster of 260 (U)/100 (Yb) atoms in the presence of a core-hole (U)/RPA (Yb) [4]. The exchange correlation Hedin-Lundquist potential was employed, reducing the 2p3/2 core-hole lifetime broadening (U: 8.1 eV, Yb: 4.3 eV) to 2.8 eV (U)/2 eV (Yb) and correcting the Fermi energy by -1 eV (U)/-8 eV(Yb). Full MS calculations were done on a cluster of 250 (U)/100 (Yb) atoms. Dipole (2p3/2→5d/6d) and quadrupole transitions (2p3/2→4f/5f) were taken into account. The Yb L3-CC-RIXS calculations were performed by using the RIXS card (see [6]).  3. Results and discussion The calculated spectra of Yb L3-HR-XANES, L3-CC-RIXS of Yb2O3 and U L3-HR-XANES, U unoccupied f and d angular momentum projected density of states (d and f-DOS) of schroeckingerite are plotted in figure 1 a, b and figure 2 d. The FEFF9.5 code successfully reproduces all spectral features at correct energy positions for U and at positions differing within few eVs from the experiment for Yb; some intensity differences are also observed. Yb2O3 characterises with Yb1 and Yb2 sites in octahedral and distorted octahedral local coordination environment, respectively (ICSD 163730). The weighted Yb1 and Yb2 calculated spectra including only dipole or quadruple transitions are shown in figure 1 a. The Yb L3-HR-XANES spectrum is a linear combination of the two calculated spectra (1/4 Yb1 and 3/4 Yb2). The A region from the pre-edge structure originates mainly from 2p3/2→4f electronic transitions but 2p3/2→5d transitions are also well distinguishable. The energy difference between features A and B2 (13.4 eV) is equal, whereas between B1 and B2 (2.8 eV) and B2 and C (12.1 eV) is smaller than in the experimental spectrum (B2-A=13.4 eV, B2–B1=3.3 eV, C-B2=16.7 eV). The Yb Lα1 on the energy transfer scale is plotted as a function of the excitation energy in figure 1 b (Yb L3-CC-RIXS). The Yb2O3 L3-CC-RIXS has intense pre-edge structure at about 8935 eV and a double structure in the WL region. The left RIXS plot shows the FEFF9.5 calculation result using only dipole transitions (2p3/2→5d), the middle plot the result obtained including quadrupole 15th International Conference on X-ray Absorption Fine Structure (XAFS15) IOP PublishingJournal of Physics: Conference Series 430 (2013) 012117 doi:10.1088/1742-6596/430/1/0121172      transitions (2p3/2→4f). The pre-edge absorption resonance is weak in the left plot (not visible on this scale) but has higher intensity and position comparable to the experimental spectrum (right) in the middle plot suggesting 2p3/2→4f dominates but mixes with 2p3/2→5d transitions in this part of the spectrum. This result partially confirms previous atomic multiplet calculations attributing the pre-edge to 2p3/2→4f electronic transitions, which however calculated only the pre-edge structure [2]. In case of uranium, 2p3/2 electronic transitions to 5f valence states contribute to the pre-edge region at about -9 eV, as at this energy the U f-DOS has large intensity (see figure 2 d). The WL and post-edge regions of the U L3-HR-XANES spectrum is well described by dipole 2p3/2→6d transitions and resemble the U d-DOS as expected.  We use two U(VI) minerals, meta-autunite and schroeckingerite, to compare the structural sensitivity of U M4/L3-HR-XANES and U L3-VB-RIXS spectra. Meta-autunite and schroeckingerite possess tetragonal (P4/nmm) (ICSD 20378) and triclinic (P -1) (AMCSD 0015705) crystal structures, respec-tively. In both mineral phases U(VI)O22+ dioxo cations are coordinated solely by O atoms in the equatorial plane (figure. 2c,g). Second coordination neighbours are P/O atoms (meta-autunite) or C atoms (schroeckingerite). In figure 2a, the meta-autunite and schroeckingerite U L3-HR-XANES spectra (2a top) are compared to their conventional fluorescence XANES spectra (2a bottom). All U L3-HR-XANES features are sharper than in the conventional XANES and an additional pre-edge feature A is resolved. The U M4-HR-XANES of these minerals also exhibit significantly improved energy resolution (figure 2f) which is shown here for schoepite where the distinct fine structure in the M4-HR-XANES, is not resolved in the conventional fluorescence XANES (figure 2e). Only subtle differences between the mineral phases are observed in their U M4-HR-XANES spectra such as the energy shift of feature D (figure. 2f inset). In contrast, the different U coordination environments in these mineral structures are clearly reflected in distinct variations of their U L3-HR-XANES features. The An M4,5-edges are of special interest as they directly probe unoccupied An 5f electronic state densities (3d→5f transitions) and potentially can reveal subtle bonding differences such as metal-to-ligand charge donation. In addition, An M4-XANES is expected to be especially useful for An speciation, since the reduced core-hole life-time broadening at the M4 edge compared to the L3 edge theoretically sharpens spectral features, thereby facilitating detection of minority valence species in oxidation state mixtures. However, our results on these two minerals indicate that the An L3 edge might be more sensitive to changes in coordination environment for the same An oxidation state. For example, feature C in the U L3-HR-XANES spectrum is an indicator for the U-O axial distance and shifts to lower energy upon lengthening of one or both U-O axial bonds [1]. The longest U-O axial distance in meta-autunite is about 0.2 Å longer than in schroeckingerite; however, feature C does not shift detectable to lower energies (figure. 2a). The U L3-HR-XANES spectrum of schroeckingerite is calculated by elongation of the U-O1 bond from 1.8 to 2.5 Å compared to the spectrum of the unmodified structure in figure 2 h. Moreover, the pre-edge feature A has higher intensity, whereas the intensity of the WL (feature B) decreases. This trend is also visible in the experimental spectrum of meta-autunite compared to schroeckingerite. Notice that the reduction of WL intensity is stronger in the experiment than in the calculation, suggesting influence of additional structural effects. Nevertheless, this simulation implies that features A, B and C in L3-HR-XANES can assist characterizing U-O bond distances more effectively than conventional XANES or M4-HR studies.  Figure 1 b shows the U L3-VB-RIXS spectra on the energy transfer scale of meta-autunite and schroeckingerite measured at an excitation energy at the maximum of the U L3-HR-XANES WL (17176 eV). The intense peak at 0 eV is due to the elastically scattered incident photons. In the final state, the excited U atom has an electron promoted to an empty 6d states and a core-hole in the filled part of the VB; this mimics a direct excitation from the VB [7]. Therefore, the U L3-VB-RIXS spectrum, with maximum at about 12.7 eV, describes unoccupied 6d states. The energy difference between the elastic peak and the VB-RIXS spectrum measures the energy gap between the highest occupied state and the lowest unoccupied valence state [7]. The U L3-VB-RIXS of meta-autunite exhibits a broader VB feature compared to schroeckingerite, suggesting a larger energy spread of 6d states and maybe less mixing with ligand valence orbitals. Comparison of the U L3-HR-XANES WL 15th International Conference on X-ray Absorption Fine Structure (XAFS15) IOP PublishingJournal of Physics: Conference Series 430 (2013) 012117 doi:10.1088/1742-6596/430/1/0121173      areas, which is proportional to the oscillatory strength of 2p2/3 electronic transitions to U 6d states, corroborates this interpretation; the U d states in the U L3-HR-XANES of meta-autunite have larger energy spread than schroeckingerite. Attempts to quantify this difference by fitting the U L3-HR-XANES remain unsuccessful, as no unique model using Pseudo Voigt functions was found.   Figure 1. (a) Yb L3-HR-XANES and calculation, (b) calculation including dipole (left) or dipole and quadrupole (middle) transitions, Yb L3-CC-RIXS (right) of Yb2O3.   Figure 2. (a) U L3-HR and -XANES, (b) U L3-VB-RIXS, 3.6 Å atomic cluster for schroeckingerite (c) and meta-autunite (g), (d) U L3-HR-XANES and (h) calculation for schroeckingerite, (e) U M4-HR and -XANES for schoepite, (f) U M4-HR-XANES of meta-autunite and schroeckingerite. 4. Conclusions The FEFF9.5 code emerges as a very useful tool for calculations of An/Ln L3-HR-XANES and RIXS spectra, as it successfully reproduces all spectral features in both. The U(VI) L3-HR-XANES spectra tend to be more sensitive to changes in geometric structure compared to U M4-HR-XANES and VB-RIXS for the same U oxidation state. However, the techniques are complimentary and coupled to ab initio quantum chemical calculations provide detailed geometric and electronic structural information, which, e.g., can help to explain reduction mechanisms of Ln(III) to Ln(II) and can also be valuable for understanding the selectivity of N-donor ligands to complex An(III) over Ln(III) ions relevant for the separation and transmutation strategy for reduction the radiotoxicity of spent nuclear fuel.   Acknowledgments: We gratefully acknowledge KIT and the Helmholtz Association of German Research Centers for the financial support (VH-NG-734). We thank ESRF and ANKA for the granted beamtime.   References [1] Vitova T et al. 2010 PRB 82 235118  [2] Kvashnina K O, Butorin S M and Glatzel P 2011 J. Anal. At. Spectrom. 26 1265 [3] Glatzel P and Bergmann U 2005 Coord. Chem. Rev.  249 65 [4] Rehr J J, Kas J J, Prange M P, Sorini A P, Takimoto Y and Vila F 2009 C. R.  Physique 10 548 59 [5] Rothe J et al. 2012 Rev. Sci. Instrum. 83 043105 [6] Kas J J, Rehr J J, Soininen J A, and Glatzel P 2011 PRB 83 235114  [7] Glatzel P, Singh J, Kvashnina K O and van Bokhoven J A 2012 JACS 132 2557 15th International Conference on X-ray Absorption Fine Structure (XAFS15) IOP PublishingJournal of Physics: Conference Series 430 (2013) 012117 doi:10.1088/1742-6596/430/1/0121174

Actinide and lanthanide speciation with high-energy resolution X-ray techniques

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Actinide and lanthanide speciation with high-energy resolution X-ray techniques

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