Database of ab initio L-edge X-ray absorption near edge structure

The L-edge X-ray Absorption Near Edge Structure (XANES) is widely used in the characterization of transition metal compounds. Here, we report the development of a database of computed L-edge XANES using the multiple scattering theory-based FEFF9 code. The initial release of the database contains more than 140,000 L-edge spectra for more than 22,000 structures generated using a high-throughput computational workflow. The data is disseminated through the Materials Project and addresses a critical need for L-edge XANES spectra among the research community. Measurement(s) near-edge X-ray absorption fine structure spectroscopy • L-edge XANES Technology Type(s) X-ray absorption spectroscopy Measurement(s) near-edge X-ray absorption fine structure spectroscopy • L-edge XANES Technology Type(s) X-ray absorption spectroscopy Machine-accessible metadata file describing the reported data: https://doi.org/10.6084/m9.figshare.14233055


Background & Summary
X-ray absorption spectroscopy (XAS) is a robust and valuable characterization technique for accurate identifications of atomic local environments 1 , oxidation states 2 , and electronic structures 3 , etc. In XAS, core electrons are excited after the absorption of X-ray photons. The edge names are based on the principal quantum number of the electrons excited: K for 1 s, L for 2 s or 2p,etc. The XAS can be further divided into the X-ray absorption near edge structure (XANES) and the extended X-ray absorption fine structure (EXAFS) by energy range. The XANES region often has stronger signal and can be directly correlated with atomic local environments and oxidation states of the absorbing atoms by comparing to known reference spectra. Unfortunately, the availability of reference XANES data is typically less than other X-ray based characterization techniques due to its reliance on high-energy synchrotron sources.
Researchers confront such deficiencies by gathering data from the community to construct calibrated databases 4 . For example, the EELS database (EELS DB) 5 hosted by the European Microscopy Society contains several hundred spectra covering 35 elements. More recently, Diamond Light Source has integrated data processing and collection to improve traceability 6 . In addition, researchers are establishing international collaborations to further enhance XAS data distribution and sharing 6,7 .
As a complementary alternative to experimental XAS databases, computational XAS databases are attracting increasing interest. Codes based on multiple scattering 8,9 , multiplet 10 and Bethe-Salpeter equation [11][12][13][14] methodologies are commonly used in computing the XAS. Unlike semi-empirical multiplet calculations that impose strong restrictions on symmetry options, ab initio techniques based on the Bethe-Salpeter equation and multiple scattering are able to account for deviations from the idealized coordination environment around the absorbing atom. Previously, the present authors have used the FEFF9 multiple scattering code 8 to generate the world's largest computational database of K-edge XANES spectra, the XASdb 15,16 . The XASdb currently hosts more than 500,000 K-edge XANES spectra for more than 51,000 materials, while most experimental databases only contain several hundred. The XASdb has already been extensively used in many works, including the development of machine learning models to accelerate the interpretation of XAS. For example, Zheng et al. 17 applied random forest models to predict coordination environment labels using XANES spectra from the XASdb. Andrejevic et al. 18 demonstrated that neutral network-based models are capable of classifying topological materials solely from XANES spectra by training the models on XASdb. Both works delivered >80% average accuracy among dozens of absorbing elements. Specifically for 3d transition metal elements, researchers have adopted related data from XASdb to predict coordination numbers, Bader charges, mean nearest neighbor distances 19 and local coordination environments 20 .
In this work, we further extend the XASdb by developing a database of L-edge XANES using the FEFF9 8 code. The L-edge is especially useful in the study of transition metal elements where the K-edge energies are too high for facile measurements. For instance, the L-edge XANES has been routinely used to investigate how strain, ligand, and particle size affect the performance of catalysts 21 . The L-edge XANES can be further divided into L 1 and L 2,3 edges. The L 1 -edge representing quadrupole transitions is typically broadened, weak and lacks significant information for interpretation 22 . Thus our focus is on the L 2,3 -edge derived from intense dipole-allowed transitions. Our L-edge XANES database covers around 140,000 L 2,3 -edge XANES for more than 22,000 structures. It has been integrated as part of the XASdb hosted on the Materials Project 23 website for individual spectrum visualization and download. A complete set of L-edge data can be downloaded separately in JSON format. This L-edge dataset serves as a reliable repository of reference spectra and enables machine learning applications using L-edge data.

theory.
In the perspective of computational XAS, Fermi's golden rule governs the transition probability for a given initial state i and final state f . This transition rate is proportional to X-ray absorption coefficient, and can be expressed in terms of the wavefunction as follows: where ψ i and ψ f are the initial and final eigenstates, and A(r) · p accounts for the coupling of X-ray field. The L 2,3 -edge XANES is due to 2p-to-nd transitions. If written in terms of the one-particle Green's function, µ can be calculated in a more efficient way using the following equation: where the ε ⋅ r is the interaction operator in dipole approximation. G r r E ( , ; ) can be further divided into the contribution from the central atom, G c and the contribution from the remaining scatters G sc (see ref. 8 and references therein). This theoretical formalism is implemented in the ab-initio real-space multiple-scattering XAS code FEFF9 for general calculations of X-ray spectra throughout the periodic table 8 . For a more thorough background in the theory, we direct the interested readers to the review paper by Rehr et al. 24 .
High-throughput workflow. A high-throughput workflow for L-edge calculations was developed using pymatgen 25 , FireWorks 26 and atomate 27 , as shown in Fig. 1.
The initial input structure is obtained from relaxed structures in the Materials Project 23 database. For each symmetrically distinct site within the structure, a site-wise spectrum is computed with automatic convergence checks and error recovery using the custodian package 28 . Then the raw site-wise spectra are averaged www.nature.com/scientificdata www.nature.com/scientificdata/ to element-wise spectra based on site multiplicity and inserted into the XASdb, which can be accessed via the Materials Project website.
At the present moment, only structures in the Materials Project that originated from the Inorganic Crystal Structure Database (ICSD) 29 , i.e., likely to have been experimentally synthesized previously, have been calculated. Further, only elements with atomic number larger than 20 are included because the characterization of lighter elements are typically based on the K-edge XANES.
Data analysis. The cosine similarity is used to evaluate the similarity between spectra quantitatively 30 . It is defined in Eq. 3 as: where → I A and → I B represent intensity vectors for the two spectra. It was computed using the scikit-learn 31 package.

Data Records
To date, approximately 140,000 site-wise L 2 and L 3 spectra have been computed, which correspond to 40,000 site-averaged L 2,3 -edge XANES spectra for unique crystals. The data distribution for the L-edge XANES dataset is shown in Fig. 2.
Data visualization. The L-edge data were integrated with the previous K-edge data for a comprehensive display of XAS spectra on Materials Project website (https://materialsproject.org/xas). The website allows users to compare the XANES spectra interactively for K, L 2,3 , L 2 and L 3 -edge XANES spectra although L 2,3 functionality is only supported for absorbing elements with 21 ≤ Z ≤ 30. Users can also apply Gaussian smoothing to the spectra on-the-fly to account for instrumental broadening.
Data download. The dataset can be downloaded in two ways. For users interested in specific chemical systems (e.g., searching for reference spectra within Ni-O system), an API query (https://api.materialsproject.org/ docs#/XAS) through the representational state transfer (REST) endpoint interfaced with the XASdb is recommended. The data obtained through API are site-averaged spectra, which can be directly compared to experimental spectra. The second method is to download a L-XAS.json.tgz file for a complete set of site-wise L-edge data through figshare (https://doi.org/10.6084/m9.figshare.12824513.v1) 32 . The complete dataset is appropriate for data-intensive applications such as machine learning. The detailed data structure is shown in Table 1.

technical Validation
We performed validation of FEFF9's input parameters based on a comparison between computational and experimental spectra. Unlike the previous K-edge database works 15,16 that covered a more thorough benchmark on FEFF9 input parameters, only critical input parameters that shape the L-edge spectrum, such as the cluster radius in self-consistent field (SCF) calculations and the core-hole treatment, are discussed here. A more detailed discussion about the full multiple scattering (FMS) calculations and the choice of exchange correlation potential, which are kept the same for the L-edge calculations, can be found in previous works on the K-edge calculations 15,16 www.nature.com/scientificdata www.nature.com/scientificdata/ for interested readers. While more advanced treatments such as Debye-Waller factors can be performed using FEFF9, we did not benchmark them in this high-throughput work. A total of 18 experimental reference spectra were collected and listed in Table 2. We included diverse absorbing species (both 3d transition metal and heavy 4 f absorbing species) and various local environment to unveil a convergent set of inputs.
The cluster radius in SCF calculations determines the number of atoms to be included in the coordination shell. A sufficiently large cluster radius is necessary to account for all scattering effects but an excessively large one will cause an increase in computation cost and an overestimation of multiple scattering from long-distance atoms 33 . From Fig. 3, we found that a cluster radius of 5.5 Å was sufficient to converge the L-edge spectra to a cosine similarity of 0.98 compared to a cluster radius of 8 Å.
Another important input parameter to FEFF9 calculations is the core-hole treatment. When the core electron is excited by X-ray photons, it creates a photon-electron or core-hole pair. Among all three core-hole treatments supported by FEFF9, i.e., the final state rule (FSR), the random phase approximation (RPA) and no core-hole (NONE), it was found that calculated spectra without core-hole treatment resulted in the best agreement (highest cosine similarity) with experiments, as shown in Fig. 3. FSR sometimes breaks down for L-shell calculations while RPA can cause an irregular shake-up in the post-edge region of the XANES spectrum. Further, the more mobile electrons at outer shells (e.g., 2p vs. 1 s electrons) lead to stronger screening of the core-hole effect than can be accounted for with FSR or RPA.
In Fig. 4, the spectra calculated using the FEFF9 converged input parameters are compared against experimental spectra as well as spectra computed using ocean 11,12 , an alternative software based on the Bethe-Salpeter equation for XANES calculation. A horizontal shift to align the L 3 peak and a Gaussian broadening with full width at half maximum (FWHM) of 1.2 eV were applied to the computed spectra to account for the less accurate determination of Fermi level and the instrumental broadening, respectively. In general, the FEFF9 spectra are in relatively good agreement with experimental measurements and the ocean computed spectra in terms of relative peak positions and peak intensities. For Ti in rutile TiO 2 and V in α-V 2 O 5 , the L 2 peak intensities and the edge separation computed by ocean are in better agreement with experiments than FEFF9, which can be explained by  www.nature.com/scientificdata www.nature.com/scientificdata/ the inclusion of spin-orbit coupling during ocean calculation. However, the significantly higher computational costs and poorer scalability of ocean calculations make it less suitable for high-throughput generation of spectra.
The L 2,3 -edge XANES spectra for eight 3d transition metal elements in various crystals are plotted in Fig. 5. These elements are predominantly in the octahedral and tetrahedral local environments 34 . Except for Ti and Mn where the octahedral environment dominates, the rest of the 3d transition metals have a more even distribution of octahedral and tetrahedral local environment. The L 3 /L 2 branching ratio, defined as the ratio of integrated intensities for L 3 and L 2 peaks, is vital to the spin states because this property is proportional to the number of paired electrons. In theory, the branching ratio for an absorbing atom in tetrahedral environment is smaller than that in octahedral environment. The crystal field splitting for tetrahedral environment is smaller than that of octahedral environment, leading to a preference for high-spin states over low-spin states in the tetrahedral environment. This is consistent with the observation that the L 2 peak intensities for 3d transition metals such as Mn, Fe, Co, Ni and Fig. 3 Benchmarking results for (a) cluster radius for SCF, and (b) core-hole treatment parameters for FEFF9 L-edge XANES calculations. When benchmarking cluster radius for each chemical system, the cosine similarities are computed with respect to the spectrum that is calculated with a cluster radius of 8 Å. A comparison between L 2,3 -edge XANES is conducted for all absorbing elements except the heavy 5f elements Ce and Pt. For Ce and Pt, only the L 3 -edge XANES are compared because of large energy separation between the L 2 and L 3 peaks. For core-hole treatment, the cosine similarities are calculated between the computed spectra and experimental spectra for all chemical systems listed in Table 2. Fig. 4 Comparison between experimental spectra, ocean computed spectra and FEFF9 computed spectra. The first and second major peaks are the L 3 and L 2 peak, respectively. The third peak in experimental V L-edge spectrum in α-V 2 O 5 , indicated by the black dashed rectangle, is contributed by the oxygen K-edge, which is not accounted for in the computed spectra. The details of experimental data can be found in Table 2. Spectra are shifted vertically and normalized to maximum intensity for ease of visualization. ( www.nature.com/scientificdata www.nature.com/scientificdata/ Cu in tetrahedral environment are significantly larger than in the octahedral environment. Another important finding comes from the decrease of white-line intensities. The white line refers to the intense absorption in the rising edge region of a XANES spectrum. Its intensity is positively related to the number of unoccupied d states. With increasing number of valence states, the white line intensities continue to decrease along with filling of d orbitals. While most FEFF spectra trends are consistent with theory, we observed that a small number of spectra (53 out of around 140,000 site-wise spectra) possess unphysical negative intensities. This could be caused by the instability when directly solving the complex Green's function, which leads to small negative spectra weight since the phase might be wrong. Another possible explanation lies in the numerical precision differences between the atomic background and the scattering contributions, which are calculated separately. While extra caution is needed, it is up to users and use cases to determine how to treat those spectra with negative intensities.

Usage Notes
Each entry in the database contains site-specific or site-averaged L-edge XANES (as well as K-edge XANES), together with physical and chemical properties such as the elemental oxidation states and coordination environments. These data can be used as references for comparison with experimental spectra to identify the properties of species present or local environment when using a very fine electron energy loss spectroscopy (EELS) probe. While there are discrepancies between the computed and experimental spectra for certain elements (especially the early transition metals), this can be mitigated through computations with other high-level codes such as ocean for select systems.
Another potential usage of this dataset is in the development of machine learning (ML) models to accelerate spectra interpretation. ML models such as random forest 17,19 and neural networks 18,20 have been developed using our previously-constructed K-edge XANES database, with accuracies exceeding 80% having been achieved in classifying the local environment. Potentially, similar or more refined ML models, especially for transition metal systems, can be developed using both the K-edge and L-edge XANES. For instance, the branching ratio in L 2,3 -edge XANES can be used to distinguish between different spin states even in the same complexes 35 .
In summary, a large dataset covering 140,000 L 2,3 -edge XANES spectra are made open to the public after an in-depth benchmark, complementing the world's largest computational XAS database. Our benchmark results indicate that multiple scattering codes such as FEFF9 can achieve comparable accuracy when compared to experimental data. We anticipate this work to benefit the whole XAS community through well-curated data and elaborated dissemination.

Code availability
The workflow for FEFF9 calculation including input generation, output parsing and workflow management is available in open-source materials science packages pymatgen 25 , FireWorks 26 and atomate 27 . The error handler for automatic error detection and recovery can be found in custodian 28 .