research communications
2Sr[Fe(CN)6], from laboratory X-ray powder data
of dicaesium strontium hexacyanidoferrate(II), CsaCEA, DES, ISEC, DE2D, Univ Montpellier, Marcoule, France, bKazuo Inamori School of Engineering, Alfred University, Alfred, NY, 14802, USA, and cCenter for Hierarchical Waste Form Materials, Columbia, SC, 29208, USA
*Correspondence e-mail: nicolas.massoni@cea.fr
Ferrocyanides with general formula AIxBIIy[Fe(CN)6], where A and B are cations, are thought to accept many substitutions on the A and B positions. In this communication, the synthesis and of Cs2Sr[Fe(CN)6] are reported. The latter was obtained from K2Ba[Fe(CN)6] particles, put in contact with caesium and strontium ions. Hence, a simultaneous ion-exchange mechanism (Cs for K, Sr for Ba) occurs to yield Cs2Sr[Fe(CN)6]. The synthesis protocol shows that K2BaFe(CN)6 particles can be used for the simultaneous trapping of radioactive caesium and strontium nuclides in water streams. Cs2Sr[Fe(CN)6] adopts the cryolite structure type and is isotypic with the known compound Cs2Na[Mn(CN)6] [dicaesium sodium hexacyanidomanganate(III)]. The octahedrally coordinated Sr and Fe sites both are located on inversion centres, and the eightfold-coordinated Cs site on a general position.
Keywords: crystal structure; X-ray powder diffraction; caesium strontium hexaferrocyanate; cryolite-type structure.
CCDC reference: 2004551
1. Chemical context
Ferrocyanides (FCN), such as Prussian blue, were discovered almost 300 years ago. The attractive properties of these materials for batteries and decontamination processes have ensured that FCNs remain an active research topic (Haas, 1993; Paolella et al., 2017). In particular, potassium copper FCN is currently being investigated for the purification of 137Cs-contaminated water streams through partial exchange with potassium (Haas, 1993; Mimura et al., 1997). To the best of our knowledge, however, using FCNs to extract strontium either alone or with caesium has never been considered before. In the framework of the Center for Hierarchical Waste Forms (CHWM), an Energy Frontier Research Center (EFRC) funded by the US Department of Energy, we have been working on potassium copper FCN as an efficient K-ionic exchanger to capture 137Cs and serve as a waste containment matrix (zur Loye et al., 2018). In this context, we have synthesized a cesium strontium FCN to study its efficiency in immobilizing both 90Sr and 137Cs, two radionuclides that are in most cases found together in radioactive water streams. Caesium strontium FCNs appear to be poorly described in the ICDD 2020 PDF4+ powder diffraction database (Gates-Rector & Blanton, 2019). Since the synthesized phase Cs2Sr[Fe(CN)6] did not match with existing entries, we decided to characterize the structure and we report the results herein.
2. Structural commentary
Cs2Sr[Fe(CN)6] is isotypic with Cs2Na[Mn(CN)6] (Ziegler et al., 1989). As shown in Table 1, the lattice parameters of Cs2Sr[Fe(CN)6] are slightly greater than those of Cs2Na[Mn(CN)6], but the cell volumes differ by less than 0.3%. The adopts the cryolite structure type and comprises a framework of corner-sharing [Sr(CN)6] (dark green in Fig. 1) and [Fe(CN)6] octahedra (brown in Fig. 1). Both types of octahedra exhibit , with Sr situated on 2 c, and Fe on 2 a. In the voids of this framework, Cs sites (light green in Fig. 1) have a distorted square-antiprismatic environment with four C and four N atoms as ligands. The substitution of manganese by iron in Cs2Na[Mn(CN)6] can be explained by the similar ionic radii of the two elements: rMn(III) = 0.58 Å and rFe(II) = 0.61 Å (Shannon, 1976). For the substitution of sodium by strontium, the ionic radii differ more substantially: rNa(I) = 1.02 Å and rSr(II) = 1.18 Å. The two crystal structures were compared numerically using COMPSTRU (de la Flor et al., 2016). The structure similarity index Δ was calculated to be 0.009 (Bergerhoff et al., 1999). However, since only a few parameters (11) were refined and many parameters kept fixed in the the similarity index is not reliable.
3. Database survey
Ferrocyanides have rather complex structures. The ICDD 2020 PDF4+ database (Gates-Rector & Blanton, 2019) contains records of about 1521 phases with the general AIxBIIy[Fe(CN)6] ferrocyanide formula in which A and B are cations, with no constraints on the A:B ratio. As shown in Fig. 2, the studied sample contained only Cs, Sr, Fe, C and N. Hence, we focused on ferrocyanides with AI = Cs and BII = Sr, for which only three phases have been reported, however with poorly described crystal data. The Cs2Sr[Fe(CN)6] phase studied by Kuznetsov et al. (1970) is reported to crystallize in the tetragonal with a ranging from 10.72 to 10.89 Å and c from 10.75 to 10.99 Å (PDF00-024-0293 and PDF00-24-0294). The entry for the third phase (PDF00-048-1203), the hydrated ferrocyanide CsSr[Fe(CN)6]·3H2O reported by Slivko et al. (1988), is comprised only of reflections without further crystal data given. None of these PDF cards matched the X-ray diffraction pattern of the studied sample. As shown in Fig. 2a,b, the cubic revealed by SEM measurements hints at a with cubic symmetry, but the number of reflections is not consistent with such a highly symmetrical The whole pattern can be described by a monoclinic cell and the experimental data are well reproduced by adjusting the reflections from the Cs2Na[Mn(CN)6] phase (Ziegler et al., 1989; PDF 04-012-3126). The Cs2Sr[Fe(CN)6] was refined from that of Cs2Na[Mn(CN)6] assuming complete substitution of manganese by iron and sodium by strontium. As described above, the ionic radii of the corresponding metals are close enough for these substitutions to be possible.
4. Synthesis and crystallization
All solutions were prepared using Millipore water. Cs2Sr[Fe(CN)6] (Cs2SrHCF) particles were not prepared directly by adding Sr and Cs salts to K4[Fe(CN)6]·3H2O. Although it was found that Cs2SrHCF could be prepared directly by adding aqueous Sr(NO3)2 to a K4[Fe(CN)6]·3H2O/CsNO3 solution, the yield was extremely poor (≤ 1%). Instead, an ion-exchange reaction was initiated by adding a mixed Sr(NO3)2/CsNO3 solution to K2Ba[Fe(CN)6] particles, thereby simultaneously substituting barium for strontium and potassium for cesium. This simple approach, using K2Ba[Fe(CN)6]·2.6H2O (K2BaHCF) as an intermediate compound, allowed 1:1 amounts of Cs2SrHCF to be produced from K2BaHCF by ion exchange.
Briefly, the K2BaHCF itself was prepared by adding a 1.5 M solution of Ba(NO3)2 to a 1 M solution of K4[Fe(CN)6]·3H2O as described by Padigi et al. (2015). Once prepared, K2BaHCF was collected by centrifugation, washed and dried. Its chemical composition (K, Fe and Ba) and water content, respectively, were determined by inductively coupled plasma (ICP) analysis and thermogravimetric analysis (TGA). The dried K2BaHCF particles redispersed readily in water, producing a clear, slightly yellow dispersion. Cs2SrHCF forms immediately as a milky white precipitate (Fig. 3a) upon adding the mixed CsNO3/Sr(NO3)2 solution to the clear yellow K2BaHCF dispersion. To ensure complete substitution, 2.2 moles of CsNO3 and 1.1 moles of Sr(NO3)2 were added for every mole of K2BaHCF present. After being left to mix for 1 h, the formed Cs2SrHCF was collected by centrifugation, washed and dried. The chemical composition (Fe and Sr) of the powder was determined by ICP analysis while the Cs content was determined by atomic absorption spectroscopy (AAS). An initial characterization of the Cs2SrHCF powder was carried out by TGA, UV–Vis and FT–IR spectroscopy. The UV–Vis spectrum of the Cs2SrHCF (Fig. 3b) confirmed that the [Fe(CN)6] moiety was maintained with only slight decreases in the wavelengths of the various absorption peaks (Gray & Beach, 1963). The FT–IR spectra of Cs2SrHCF and K2BaHCF are shown in Fig. 3c. While a δ(HOH) signal is observed for K2BaHCF at 1611 cm−1 along with ν(OH) signals at 3527 cm−1 and 3601 cm−1, no such signals were detected for Cs2SrHCF. This absence of water was confirmed by TGA, which showed no mass loss between 30 and 400°C (Fig. S1 in the supporting information. The largest change was in the ν(M—N) stretching mode, which shifted from 421 cm−1 ν(Ba—N) to 439 cm−1 ν(Sr—N) (Fig. 3d).
5. Refinement
Crystal data and details of the data collection and structure . The observed and calculated intensities are shown in Fig. 4 along with the difference pattern. For the of Cs2Sr[Fe(CN)6], atomic positions of the Cs2Na[Mn(CN)6] phase (Ziegler et al., 1989) and the given individual isotropic displacement parameters were used. All occupancies were set to unity because of the experimentally determined composition. Except for cesium, all displacement parameters were kept fixed because otherwise some became negative. The positions of the nitrogen and carbon atoms were also kept fixed. Since iron and strontium atoms are in special positions, only the lattice parameters, the position of the cesium atom and its Uiso value were refined, together with three profile parameters. The residual electron density is about is 6.06 e Å−3 at a distance of 0.71 Å from Cs.
methods are summarized in Table 2
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Supporting information
CCDC reference: 2004551
https://doi.org/10.1107/S2056989020006660/wm5555sup1.cif
contains datablocks cacesio, I. DOI:TG curves of Cs2Sr[Fe(CN)6] and K2Ba[Fe(CN)6].2.6H2O. DOI: https://doi.org/10.1107/S2056989020006660/wm5555sup2.png
Data collection: Data Collector (Panalytical, 2011); cell
JANA2006 (Petříček et al., 2014); data reduction: JANA2006 (Petříček et al., 2014); program(s) used to solve structure: coordinates from isotypic compound; program(s) used to refine structure: JANA2006 (Petříček et al., 2014); molecular graphics: VESTA (Momma & Izumi, 2011); software used to prepare material for publication: publCIF (Westrip, 2010).Cs2Sr[Fe(CN)6] | F(000) = 504 |
Mr = 565.4 | y |
Monoclinic, P21/n | Dx = 2.885 Mg m−3 |
a = 7.6237 (2) Å | Cu Kα1 radiation, λ = 1.540562, 1.544390 Å |
b = 7.7885 (2) Å | T = 293 K |
c = 10.9600 (3) Å | Particle morphology: plate-like |
β = 90.4165 (19)° | brown |
V = 650.76 (4) Å3 | flat_sheet, 25 × 25 mm |
Z = 2 | Specimen preparation: Prepared at 1873 K and 100 kPa, cooled at 30 K min−1 |
Panalytical XPert MPD Pro diffractometer | Data collection mode: reflection |
Radiation source: sealed X-ray tube | Scan method: step |
Specimen mounting: packed powder pellet | 2θmin = 10.023°, 2θmax = 130.010°, 2θstep = 0.017° |
Rp = 0.031 | 11 parameters |
Rwp = 0.043 | 0 restraints |
Rexp = 0.025 | 26 constraints |
R(F) = 0.101 | Weighting scheme based on measured s.u.'s |
6881 data points | (Δ/σ)max = 0.012 |
Profile function: Lorentzian | Background function: Manual background |
Refinement. The Platon test reports 21 Alerts level C. They could be gathered in three groups for explanation : i)17 C-Alerts (out of 21) are "missing esd on x,y,z coordinates of N and C atoms. This is normal since these positions were not refined. Hence no esd was calculated by Jana2006. ii)3 C-Alerts (out of 21) are due to a slighlty larger Fourier difference density than allowed by CheckCIF. I can not enhance the quality of the data so no reduction of this value can be done. iii) The last C-Alert is about a "calc. and reported Sum Formula which differ. I did not find the origin of the Alert. |
x | y | z | Uiso*/Ueq | ||
Cs | 0.5080 (4) | −0.04022 (18) | 0.2497 (7) | 0.0410 (6)* | |
Sr | 0 | 0 | 0.5 | 0.024* | |
Fe | 0 | 0 | 0 | 0.019* | |
C1 | 0.0488 | 0.0087 | 0.178 | 0.029* | |
N1 | 0.0754 | 0.0169 | 0.2809 | 0.052* | |
C2 | −0.2128 | 0.1444 | 0.022 | 0.03* | |
N2 | −0.3347 | 0.2296 | 0.0368 | 0.048* | |
C3 | 0.1449 | 0.2097 | −0.0251 | 0.029* | |
N3 | 0.2281 | 0.3301 | −0.0406 | 0.046* |
U11 | U22 | U33 | U12 | U13 | U23 | |
Cs | 0.0576 (17) | 0.0343 (13) | 0.0345 (16) | −0.016 (4) | 0.0050 (17) | −0.008 (4) |
Cs—C1 | 3.603 (3) | Sr—N3i | 2.4965 (1) |
Cs—C1i | 3.628 (2) | Sr—N3vi | 2.4965 (1) |
Cs—N1 | 3.348 (3) | Fe—C1 | 1.9845 (1) |
Cs—N1i | 3.5232 (18) | Fe—C1vii | 1.9845 (1) |
Cs—C2ii | 3.592 (6) | Fe—C2 | 1.9901 (1) |
Cs—N2ii | 3.367 (6) | Fe—C2vii | 1.9901 (1) |
Cs—C3iii | 3.711 (5) | Fe—C3 | 1.9920 (1) |
Cs—N3iii | 3.274 (6) | Fe—C3vii | 1.9920 (1) |
Sr—N1 | 2.4767 (1) | C1—N1 | 1.1462 (1) |
Sr—N1iv | 2.4767 (1) | C2—N2 | 1.1543 (1) |
Sr—N2v | 2.4857 (1) | C3—N3 | 1.1455 (1) |
Sr—N2iii | 2.4857 (1) | ||
Csi—Cs—Csviii | 89.42 (6) | N1—Cs—N3iii | 111.23 (16) |
Csi—Cs—Csix | 88.75 (4) | N1i—Cs—C2ii | 115.67 (16) |
Csi—Cs—Csx | 178.16 (6) | N1i—Cs—N2ii | 127.6 (2) |
Csi—Cs—Csxi | 94.04 (12) | N1i—Cs—C3iii | 142.4 (2) |
Csi—Cs—Csxii | 93.31 (12) | N1i—Cs—N3iii | 130.34 (17) |
Csi—Cs—Sr | 57.71 (7) | C2ii—Cs—N2ii | 18.74 (3) |
Csi—Cs—Srii | 128.17 (12) | C2ii—Cs—C3iii | 91.10 (5) |
Csi—Cs—Sri | 55.62 (7) | C2ii—Cs—N3iii | 89.11 (6) |
Csi—Cs—Srviii | 125.77 (11) | N2ii—Cs—C3iii | 85.88 (4) |
Csi—Cs—C1 | 52.06 (4) | N2ii—Cs—N3iii | 89.50 (5) |
Csi—Cs—C1i | 39.87 (4) | C3iii—Cs—N3iii | 17.47 (3) |
Csi—Cs—N1 | 52.61 (4) | Csxiii—Sr—Cs | 108.15 (11) |
Csi—Cs—N1i | 35.27 (4) | Csxiii—Sr—Csi | 67.33 (6) |
Csi—Cs—C2ii | 135.00 (18) | Csxiii—Sr—Csviii | 71.79 (7) |
Csi—Cs—N2ii | 134.15 (18) | Csxiii—Sr—Csiv | 71.85 (11) |
Csi—Cs—C3iii | 133.13 (17) | Csxiii—Sr—Csxii | 180 |
Csi—Cs—N3iii | 135.35 (19) | Csxiii—Sr—Csxiv | 108.21 (7) |
Csviii—Cs—Csix | 178.16 (6) | Csxiii—Sr—Csvi | 112.67 (6) |
Csviii—Cs—Csx | 88.75 (4) | Csxiii—Sr—N1 | 67.84 (8) |
Csviii—Cs—Csxi | 84.87 (11) | Csxiii—Sr—N1iv | 112.16 (8) |
Csviii—Cs—Csxii | 84.16 (11) | Csxiii—Sr—N2v | 55.97 (3) |
Csviii—Cs—Sr | 51.21 (7) | Csxiii—Sr—N2iii | 124.03 (3) |
Csviii—Cs—Srii | 121.54 (11) | Csxiii—Sr—N3i | 137.39 (4) |
Csviii—Cs—Sri | 123.59 (12) | Csxiii—Sr—N3vi | 42.61 (4) |
Csviii—Cs—Srviii | 53.50 (6) | Cs—Sr—Csi | 68.79 (6) |
Csviii—Cs—C1 | 40.22 (4) | Cs—Sr—Csviii | 73.18 (7) |
Csviii—Cs—C1i | 126.52 (9) | Cs—Sr—Csiv | 180 |
Csviii—Cs—N1 | 37.42 (4) | Cs—Sr—Csxii | 71.85 (11) |
Csviii—Cs—N1i | 124.14 (8) | Cs—Sr—Csxiv | 106.82 (7) |
Csviii—Cs—C2ii | 98.28 (9) | Cs—Sr—Csvi | 111.21 (6) |
Csviii—Cs—N2ii | 79.54 (8) | Cs—Sr—N1 | 41.51 (8) |
Csviii—Cs—C3iii | 73.00 (7) | Cs—Sr—N1iv | 138.49 (8) |
Csviii—Cs—N3iii | 90.47 (9) | Cs—Sr—N2v | 105.29 (4) |
Csix—Cs—Csx | 93.09 (6) | Cs—Sr—N2iii | 74.71 (4) |
Csix—Cs—Csxi | 95.39 (13) | Cs—Sr—N3i | 52.52 (6) |
Csix—Cs—Csxii | 95.81 (13) | Cs—Sr—N3vi | 127.48 (6) |
Csix—Cs—Sr | 127.44 (12) | Csi—Sr—Csviii | 109.57 (11) |
Csix—Cs—Srii | 59.69 (7) | Csi—Sr—Csiv | 111.21 (6) |
Csix—Cs—Sri | 55.27 (7) | Csi—Sr—Csxii | 112.67 (6) |
Csix—Cs—Srviii | 127.94 (12) | Csi—Sr—Csxiv | 70.43 (11) |
Csix—Cs—C1 | 138.10 (8) | Csi—Sr—Csvi | 180 |
Csix—Cs—C1i | 51.68 (4) | Csi—Sr—N1 | 61.18 (7) |
Csix—Cs—N1 | 140.75 (6) | Csi—Sr—N1iv | 118.82 (7) |
Csix—Cs—N1i | 54.06 (4) | Csi—Sr—N2v | 36.60 (5) |
Csix—Cs—C2ii | 83.13 (9) | Csi—Sr—N2iii | 143.40 (5) |
Csix—Cs—N2ii | 101.85 (11) | Csi—Sr—N3i | 70.10 (5) |
Csix—Cs—C3iii | 108.22 (12) | Csi—Sr—N3vi | 109.90 (5) |
Csix—Cs—N3iii | 90.74 (10) | Csviii—Sr—Csiv | 106.82 (7) |
Csx—Cs—Csxi | 85.93 (12) | Csviii—Sr—Csxii | 108.21 (7) |
Csx—Cs—Csxii | 86.37 (12) | Csviii—Sr—Csxiv | 180 |
Csx—Cs—Sr | 120.84 (11) | Csviii—Sr—Csvi | 70.43 (11) |
Csx—Cs—Srii | 52.95 (7) | Csviii—Sr—N1 | 51.05 (8) |
Csx—Cs—Sri | 125.72 (13) | Csviii—Sr—N1iv | 128.95 (8) |
Csx—Cs—Srviii | 52.97 (6) | Csviii—Sr—N2v | 124.75 (7) |
Csx—Cs—C1 | 126.21 (7) | Csviii—Sr—N2iii | 55.25 (7) |
Csx—Cs—C1i | 141.80 (10) | Csviii—Sr—N3i | 122.47 (4) |
Csx—Cs—N1 | 125.56 (5) | Csviii—Sr—N3vi | 57.53 (4) |
Csx—Cs—N1i | 146.56 (9) | Csiv—Sr—Csxii | 108.15 (11) |
Csx—Cs—C2ii | 45.51 (8) | Csiv—Sr—Csxiv | 73.18 (7) |
Csx—Cs—N2ii | 45.53 (9) | Csiv—Sr—Csvi | 68.79 (6) |
Csx—Cs—C3iii | 46.01 (8) | Csiv—Sr—N1 | 138.49 (8) |
Csx—Cs—N3iii | 44.55 (9) | Csiv—Sr—N1iv | 41.51 (8) |
Csxi—Cs—Csxii | 166.72 (4) | Csiv—Sr—N2v | 74.71 (4) |
Csxi—Cs—Sr | 123.46 (9) | Csiv—Sr—N2iii | 105.29 (4) |
Csxi—Cs—Srii | 126.26 (10) | Csiv—Sr—N3i | 127.48 (6) |
Csxi—Cs—Sri | 59.14 (9) | Csiv—Sr—N3vi | 52.52 (6) |
Csxi—Cs—Srviii | 50.43 (7) | Csxii—Sr—Csxiv | 71.79 (7) |
Csxi—Cs—C1 | 75.93 (12) | Csxii—Sr—Csvi | 67.33 (6) |
Csxi—Cs—C1i | 108.98 (13) | Csxii—Sr—N1 | 112.16 (8) |
Csxi—Cs—N1 | 94.11 (14) | Csxii—Sr—N1iv | 67.84 (8) |
Csxi—Cs—N1i | 90.80 (13) | Csxii—Sr—N2v | 124.03 (3) |
Csxi—Cs—C2ii | 43.39 (9) | Csxii—Sr—N2iii | 55.97 (3) |
Csxi—Cs—N2ii | 41.07 (9) | Csxii—Sr—N3i | 42.61 (4) |
Csxi—Cs—C3iii | 125.88 (9) | Csxii—Sr—N3vi | 137.39 (4) |
Csxi—Cs—N3iii | 130.40 (11) | Csxiv—Sr—Csvi | 109.57 (11) |
Csxii—Cs—Sr | 52.97 (8) | Csxiv—Sr—N1 | 128.95 (8) |
Csxii—Cs—Srii | 55.18 (8) | Csxiv—Sr—N1iv | 51.05 (8) |
Csxii—Cs—Sri | 133.85 (9) | Csxiv—Sr—N2v | 55.25 (7) |
Csxii—Cs—Srviii | 116.50 (7) | Csxiv—Sr—N2iii | 124.75 (7) |
Csxii—Cs—C1 | 100.15 (13) | Csxiv—Sr—N3i | 57.53 (4) |
Csxii—Cs—C1i | 83.65 (13) | Csxiv—Sr—N3vi | 122.47 (4) |
Csxii—Cs—N1 | 81.64 (13) | Csvi—Sr—N1 | 118.82 (7) |
Csxii—Cs—N1i | 101.55 (14) | Csvi—Sr—N1iv | 61.18 (7) |
Csxii—Cs—C2ii | 131.46 (10) | Csvi—Sr—N2v | 143.40 (5) |
Csxii—Cs—N2ii | 128.90 (10) | Csvi—Sr—N2iii | 36.60 (5) |
Csxii—Cs—C3iii | 43.02 (8) | Csvi—Sr—N3i | 109.90 (5) |
Csxii—Cs—N3iii | 42.36 (10) | Csvi—Sr—N3vi | 70.10 (5) |
Sr—Cs—Srii | 108.15 (15) | N1—Sr—N1iv | 180 |
Sr—Cs—Sri | 113.18 (5) | N1—Sr—N2v | 90.4970 (12) |
Sr—Cs—Srviii | 104.58 (4) | N1—Sr—N2iii | 89.5030 (12) |
Sr—Cs—C1 | 47.71 (5) | N1—Sr—N3i | 90.1559 (18) |
Sr—Cs—C1i | 80.76 (9) | N1—Sr—N3vi | 89.8441 (18) |
Sr—Cs—N1 | 29.36 (6) | N1iv—Sr—N2v | 89.5030 (12) |
Sr—Cs—N1i | 88.41 (8) | N1iv—Sr—N2iii | 90.4970 (12) |
Sr—Cs—C2ii | 149.38 (7) | N1iv—Sr—N3i | 89.8441 (18) |
Sr—Cs—N2ii | 130.69 (6) | N1iv—Sr—N3vi | 90.1559 (18) |
Sr—Cs—C3iii | 78.33 (11) | N2v—Sr—N2iii | 180 |
Sr—Cs—N3iii | 88.72 (14) | N2v—Sr—N3i | 89.952 (2) |
Srii—Cs—Sri | 114.82 (5) | N2v—Sr—N3vi | 90.048 (2) |
Srii—Cs—Srviii | 105.80 (4) | N2iii—Sr—N3i | 90.048 (2) |
Srii—Cs—C1 | 154.37 (18) | N2iii—Sr—N3vi | 89.952 (2) |
Srii—Cs—C1i | 91.92 (10) | N3i—Sr—N3vi | 180 |
Srii—Cs—N1 | 136.3 (2) | C1—Fe—C1vii | 180 |
Srii—Cs—N1i | 105.47 (9) | C1—Fe—C2 | 90.5021 (17) |
Srii—Cs—C2ii | 84.45 (6) | C1—Fe—C2vii | 89.4979 (17) |
Srii—Cs—N2ii | 94.42 (6) | C1—Fe—C3 | 90.4341 (12) |
Srii—Cs—C3iii | 48.54 (6) | C1—Fe—C3vii | 89.5659 (12) |
Srii—Cs—N3iii | 31.08 (4) | C1vii—Fe—C2 | 89.4979 (17) |
Sri—Cs—Srviii | 109.57 (15) | C1vii—Fe—C2vii | 90.5021 (17) |
Sri—Cs—C1 | 86.72 (10) | C1vii—Fe—C3 | 89.5660 (12) |
Sri—Cs—C1i | 50.37 (4) | C1vii—Fe—C3vii | 90.4341 (12) |
Sri—Cs—N1 | 99.12 (9) | C2—Fe—C2vii | 180 |
Sri—Cs—N1i | 33.14 (5) | C2—Fe—C3 | 90.387 (2) |
Sri—Cs—C2ii | 84.36 (13) | C2—Fe—C3vii | 89.613 (2) |
Sri—Cs—N2ii | 94.50 (16) | C2vii—Fe—C3 | 89.613 (2) |
Sri—Cs—C3iii | 163.24 (9) | C2vii—Fe—C3vii | 90.387 (2) |
Sri—Cs—N3iii | 145.89 (8) | C3—Fe—C3vii | 180 |
Srviii—Cs—C1 | 77.56 (8) | Cs—C1—Csviii | 99.91 (7) |
Srviii—Cs—C1i | 158.40 (18) | Cs—C1—Fe | 112.69 (12) |
Srviii—Cs—N1 | 86.35 (7) | Cs—C1—N1 | 68.07 (12) |
Srviii—Cs—N1i | 140.12 (19) | Csviii—C1—Fe | 103.06 (12) |
Srviii—Cs—C2ii | 44.81 (5) | Csviii—C1—N1 | 75.62 (12) |
Srviii—Cs—N2ii | 26.11 (2) | Fe—C1—N1 | 178.6228 (6) |
Srviii—Cs—C3iii | 77.49 (3) | Cs—N1—Csviii | 107.31 (6) |
Srviii—Cs—N3iii | 88.16 (4) | Cs—N1—Sr | 109.13 (13) |
C1—Cs—C1i | 91.87 (6) | Cs—N1—C1 | 93.41 (13) |
C1—Cs—N1 | 18.52 (2) | Csviii—N1—Sr | 95.82 (12) |
C1—Cs—N1i | 84.74 (7) | Csviii—N1—C1 | 86.01 (12) |
C1—Cs—C2ii | 112.70 (17) | Sr—N1—C1 | 155.5560 (16) |
C1—Cs—N2ii | 97.66 (14) | Csxiii—C2—Fe | 110.22 (4) |
C1—Cs—C3iii | 109.87 (10) | Csxiii—C2—N2 | 69.56 (4) |
C1—Cs—N3iii | 126.34 (13) | Fe—C2—N2 | 178.6331 (10) |
C1i—Cs—N1 | 89.26 (7) | Csxiii—N2—Srxv | 117.29 (5) |
C1i—Cs—N1i | 18.369 (10) | Csxiii—N2—C2 | 91.71 (5) |
C1i—Cs—C2ii | 127.70 (13) | Srxv—N2—C2 | 150.6891 (7) |
C1i—Cs—N2ii | 143.06 (18) | Csxvi—C3—Fe | 120.47 (5) |
C1i—Cs—C3iii | 124.0 (2) | Csxvi—C3—N3 | 59.13 (5) |
C1i—Cs—N3iii | 113.08 (18) | Fe—C3—N3 | 179.4092 (8) |
N1—Cs—N1i | 87.85 (6) | Csxvi—N3—Srviii | 106.31 (4) |
N1—Cs—C2ii | 127.37 (16) | Csxvi—N3—C3 | 103.40 (4) |
N1—Cs—N2ii | 110.12 (12) | Srviii—N3—C3 | 150.1635 (8) |
N1—Cs—C3iii | 96.46 (12) |
Symmetry codes: (i) −x+1/2, y−1/2, −z+1/2; (ii) x+1, y, z; (iii) x+1/2, −y+1/2, z+1/2; (iv) −x, −y, −z+1; (v) −x−1/2, y−1/2, −z+1/2; (vi) x−1/2, −y+1/2, z+1/2; (vii) −x, −y, −z; (viii) −x+1/2, y+1/2, −z+1/2; (ix) −x+3/2, y−1/2, −z+1/2; (x) −x+3/2, y+1/2, −z+1/2; (xi) −x+1, −y, −z; (xii) −x+1, −y, −z+1; (xiii) x−1, y, z; (xiv) x−1/2, −y−1/2, z+1/2; (xv) −x−1/2, y+1/2, −z+1/2; (xvi) x−1/2, −y+1/2, z−1/2. |
Cs2Sr[Fe(CN)6] | Cs2Na[Mn(CN)6] | ||
a, b, c | 7.6237 (2), 7.7885 (2), 10.9600 (3) | a, b, c | 7.597 (1), 7.806 (1), 10.950 (1) |
α, β, γ | 90, 90.4165 (19), 90 | α, β, γ | 90, 90.07 (1), 90 |
V | 650.76 (4) | V | 649.36 |
Cs polyhedron volume* | 44.56 | Cs polyhedron volume* | 44.46 |
Cs—C1 | 3.603 (4) | Cs—C1 | 3.6291 (5) |
Cs—N1 | 3.348 (4) | Cs—N1 | 3.3688 (5) |
Cs—C1i | 3.628 (3) | Cs—C1i | 3.5936 (5) |
Cs—N1i | 3.5232 (18) | Cs—N1i | 3.4920 (5) |
Cs—C2ii | 3.592 (6) | Cs—C2ii | 3.5831 (4) |
Cs—N2ii | 3.367 (6) | Cs—N2ii | 3.3839 (3) |
Cs—C3iii | 3.711 (5) | Cs—C3iii | 3.7044 (4) |
Cs—N3iii | 3.274 (6) | Cs—N3iii | 3.2840 (3) |
Sr octahedron volume* | 20.49 | Na octahedron volume* | 20.45 |
Fe octahedron volume* | 10.49 | Mn octahedron volume* | 10.47 |
*Atomic bond lengths were not compared since the positions of C, N, Fe and Sr were not refined. Volumes were calculated by VESTA V3.2.1 (Momma & Izumi, 2011). [Symmetry codes: (i) -x+1/2, y - 1/2, -z + 1/2; (ii) x + 1, y, z; (iii) x + 1/2, -y + 1/2, z + 1/2.] |
Funding information
Funding for this research was provided by: the Center for Hierarchical Waste Forms (CHWM), an Energy Frontier Research Center funded by the US Department of Energy, Office of Basic Energy Sciences, Division of Materials Sciences and Engineering under Award DE-SC0016574.
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