Literature DB >> 28437069

A New Look at the Structural and Magnetic Properties of Potassium Neptunate K2NpO4 Combining XRD, XANES Spectroscopy, and Low-Temperature Heat Capacity.

Anna L Smith1, Eric Colineau2, Jean-Christophe Griveau2, Karin Popa2, Guilhem Kauric3, Philippe Martin4, Andreas C Scheinost5, Anthony K Cheetham6, Rudy J M Konings2.   

Abstract

The physicochemical properties of the potassium neptunate K2NpO4 have been investigated in this work using X-ray diffraction, X-ray absorption near edge structure (XANES) spectroscopy at the Np-L3 edge, and low-temperature heat capacity measurements. A Rietveld refinement of the crystal structure is reported for the first time. The Np(VI) valence state has been confirmed by the XANES data, and the absorption edge threshold of the XANES spectrum has been correlated to the Mössbauer isomer shift value reported in the literature. The standard entropy and heat capacity of K2NpO4 have been derived at 298.15 K from the low-temperature heat capacity data. The latter suggest the existence of a magnetic ordering transition around 25.9 K, most probably of the ferromagnetic type.

Entities:  

Year:  2017        PMID: 28437069      PMCID: PMC5434478          DOI: 10.1021/acs.inorgchem.7b00462

Source DB:  PubMed          Journal:  Inorg Chem        ISSN: 0020-1669            Impact factor:   5.165


Introduction

The alkali and alkaline-earth ternary oxides of uranium, neptunium, and plutonium have attracted interest since the 1960s because of their exciting and intriguing electronic and magnetic properties.[1,2] In these systems with [Rn]6d15f (uranium and neptunium) and [Rn]6d05f (plutonium) electronic configurations, the 5f valence shell electrons have a large spatial extension and are close in energy to the 6d electrons, making them prone to chemical bonding, in contrast with the 4f electrons of the lanthanides, which are more core-like. This character leads to a wide range of oxidation states, between +3 and +7, and the occurrence of magnetic ordering behavior. The theoretical description of these systems appears extremely challenging, however, as the crystal field interaction is usually of the same order of magnitude as the spin–orbit coupling interaction and electronic repulsion.[3] The crystal-field interaction cannot be treated as a small perturbation of the electronic energy levels as is done for the [Xe]4f rare earths.[3] In the case of [Rn]5f1 and [Rn]5f0 electronic configurations, however, the contribution from electronic repulsion is removed, which greatly simplifies the interpretation. A number of studies have recently been reported on several sodium actinide phases because of their relevance for the safety assessment of sodium-cooled fast reactors (SFRs).[4−7] Those studies have revealed intriguing magnetic properties for the α-Na2NpVIO4[7] and Na4NpVIO5[6] compositions and have stressed the need to re-evaluate the Np(VI) crystal-field ground state. The physical and chemical properties of K2NpO4 have been investigated in the present work in an attempt to bring new insights into the complex behavior of Np(VI) phases. Nectoux et al. performed Mössbauer spectroscopy and magnetic susceptibility measurements on this phase in 1981 and reported intriguing results.[8] The authors suggested the occurrence of a first-order magnetic transition at 19.5(5) K as the Mössbauer spectra showed hyperfine splitting below that temperature, with an associated magnetic hyperfine field of 122 T, corresponding to an ordered moment of about 0.6 μB. However, their magnetic susceptibility data did not show any sign of an anomaly around 20 K, as could be expected from the Mössbauer results. Electronic structures can also be probed using X-ray absorption spectroscopy (XAS).[9] Coupling XAS measurements in the high-energy-resolution fluorescence-detection (HERFD) mode with theoretical calculations using the Anderson impurity model, Butorin et al.[9] have recently estimated the crystal field parameters and 5f occupancy in pentavalent NaUO3 ([Rn]5f1) and hexavalent Pb3UO6 ([Rn]5f0), revealing a significant covalent character of the chemical bond. The XAS data available on solid actinide compounds with a valence state higher than IV is still very scarce, however, and the relationship between XAS features and electronic density is not fully understood.[10] In this work, we have synthesized K2NpO4 and report for the first time a Rietveld refinement of its crystal structure and XANES spectrum collected at the Np-L3 edge. The relationship between local coordination environment and shape of the XANES spectrum is discussed, as well as the correlation between the edge absorption threshold of the neptunium XANES spectrum and the isomer shift value measured by 237Np Mössbauer spectroscopy.[8] Moreover, low-temperature heat capacity measurements have been performed to solve the discrepancy regarding the existence of magnetic ordering in this compound.

Experimental Methods

Sample Preparation and Characterization

K2NpO4 and K2UO4 were synthesized under oxygen flow and air by reaction between accurately weighed samples of neptunium dioxide (237NpO2, ORNL, Oak Ridge) or uranium dioxide (238UO2.10, JRC-Karlsruhe stocks) and potassium carbonate (K2CO3, >99%, Baker). The stoichiometric mixtures were heated with intermediate regrinding steps at 1093 K for 22 h and 1073 K for 5 h for the neptunium (green color) and uranium (orange color) compounds, respectively. The purity of the obtained materials was analyzed by X-ray diffraction. No secondary phases were detected. 238U is an α emitter with a very long half-life (4.47 billion years),[11] making it only weakly radioactive. 237Np decays to 233Pa by α emission with a half-life of 2.14 million years. The 233Pa daughter product is a β– emitter with a very short half-life (27 days) and significant γ dose rate (1.335 × 10–4 (mSv/h)/MBq).[11] The handling of those materials, requiring considerable safety precautions, was therefore done with limited quantities in α gloveboxes. The X-ray diffraction measurements were carried out using a Bruker D8 X-ray diffractometer mounted in the Bragg–Brentano configuration with a copper tube (40 kV, 40 mA) and a curved Ge monochromator (111), equipped with a LinxEye position-sensitive detector. The data were collected by step scanning in the angle range 10° ≤ 2θ ≤ 120° over a period of about 8 h. Structural analysis at room temperature was performed by the Rietveld method with the Fullprof2k suite.[12]

XANES

XANES measurements were performed at the Rossendorf BeamLine (ROBL)[13] of the European Synchrotron Radiation Facility (ESRF, Grenoble, France) on the K2NpO4 material. Small amounts (5–10 mg) of powdered sample were mixed with boron nitride (BN) in an argon-filled α glovebox and pressed into pellets for the measurements. The storage ring operating conditions were 6.0 GeV and 170–200 mA. A double-crystal monochromator mounted with a Si(111) crystal coupled to collimating and focusing Rh-coated mirrors was used. XANES spectra were collected at room temperature in transmission mode at the Np-L3 edge. A step size of 0.5 eV was used in the edge region. The energy E0 of the edge absorption threshold position was taken at the first inflection point of the spectrum by using the first node of the second derivative. The position of the white-line maximum was selected from the first node of the first derivative. Several acquisitions were performed on the same sample and summed up to improve the signal to noise ratio. Before the scans were averaged, each spectrum was aligned using the XANES spectrum of a metallic yttrium (17038 eV) reference foil located between the second and the third ionization chambers and measured at the same time as the sample. The ATHENA software (Version 0.9.20)[14] was used to remove the background and to normalize the spectra.

Low-Temperature Heat Capacity of K2NpO4 and K2UO4

Low-temperature heat capacity measurements were performed using thermal relaxation calorimetry[15] with a PPMS (Physical Property Measurement System, Quantum Design) instrument at applied magnetic fields B = 0 and 9 T in the temperature ranges T = 2.1–298.4 K for K2NpO4 and T = 2.0–312.4 K for K2UO4, respectively. The measurements were carried out on 22.6(5) mg of K2NpO4 material encapsulated in Stycast 2850 FT, and the heat capacity contribution of the Stycast was subtracted from the recorded data. A more detailed description of the experimental procedure, which is particularly well adapted to the study of radioactive materials, was given in ref (16). The measurement of K2UO4 was done on 33.2(5) mg of material without additional encapsulation in Stycast. The contributions of the sample platform, wires, and grease were deduced by a separate measurement of an addenda curve. Considering the accuracy of the PPMS instrument as estimated by Lashley et al.,[15] the reproducibility of the measurements, and the error introduced by the encapsulation procedure in Stycast of the radioactive neptunium material,[16] the final uncertainty was estimated to be about 1–2% in the middle range of acquisition (10–100 K) and reach about 3% at the lowest temperatures and near room temperature. Self-heating effects coming from the radioactive decay of 237Np were considered but appeared negligible. The use of Stycast is the main contributor to the uncertainties on the heat capacity and entropy values quoted hereafter. The final uncertainty for the uranium material is estimated to be about 1% from 100 to 300 K and reach about 3% at the lowest temperatures.[15]

Results and Discussion

Structural Refinement

K2NpO4 is isostructural with K2UO4 and crystallizes with tetragonal symmetry in space group I4/mmm. The structure of K2UO4 was refined recently on the basis of single-crystal data.[17] The refined cell parameters obtained in the present study, a = 4.3322(3) Å and c = 13.1881(13) Å, are in good agreement with the literature.[17] The refined atomic positions are given in the Supporting Information. A Rietveld refinement for the K2NpO4 phase is reported for the first time in this work (Figure ). The cell parameters obtained are a = 4.2973(4) Å and c = 13.144(12) Å. The refined atomic positions are given in Table and selected bond lengths in Table . In this structure, the neptunium cations are 6-fold coordinated, and the octahedra are connected by their equatorial vertices, forming sheets in the (ab) plane (Figure a). The potassium cations, in 9-fold coordination, are located between the sheets, holding them together. The NpO6 octahedra show a neptunyl type of coordination, with two short Np–O1 bonds at 1.84(1) Å in the axial direction and four long Np–O2 bonds at 2.15(1) Å in the equatorial plane (Figure b). The presence of a neptunyl configuration is quite common for hexavalent alkali-metal actinide oxide phases. It has been reported already for α-Na2NpO4 (Np–2O = 1.762(5) Å, Np–4O = 2.086(5) Å),[7] β-Na2NpO4 (Np–2O = 1.90 Å, Np–2O = 2.16 Å, Np–2O = 2.17 Å)[18] (orthorhombic in space groups Pbam and Pbca, respectively), and BaNpO4 (Np–2O = 1.89 Å, Np–2O = 2.10 Å, Np–2O = 2.20 Å)[19] (orthorhombic in space group Pbcm). The unit cell volume in K2NpO4 (242.7 Å3) is smaller than that for K2UO4 (247.5 Å3), which can be related to the decreasing ionic radius along the series of the actinide elements.
Figure 1

Comparison between the observed (Yobs, in red) and calculated (Ycalc, in black) X-ray diffraction patterns of K2NpO4 collected at room temperature (T = 295 ± 2 K). Yobs – Ycalc, in blue, is the difference between the experimental and calculated intensities. The Bragg reflection angular positions are marked in green. The inset shows an enlargement of the refinement in the angle range 2θ = 70–120°. Measurements were carried out with λ = Cu Kα1 radiation.

Table 1

Refined Atomic Positions in K2NpO4 Derived from the Analysis of the X-ray Diffraction Data Collected at Room Temperature (T = 295 ± 2 K)a

atomoxidn stateWyckoffxyzB02)
Np+62a0000.78(1)
K+14e0.50.50.1520(2)1.91(6)
O1–24e000.1415(5)1.5(2)
O2–24c0.5002.1(2)

Rwp = 13.5, Rexp = 5.37, χ2 = 6.29.

Table 2

Selected Bond Lengths in M2AnO4 (An = U, Np; M = Na, K)a

  bond length (Å)
bondNK2UO4K2NpO4α-Na2NpO4
An–O121.812(7)1.860(7)1.762(5)
An–O242.166(1)2.149(1)2.086(5)
K–O112.801(7)2.714(7) 
K–O143.068(1)3.042(1) 
K–O242.935(2)2.934(2) 

N is the number of atoms in each coordination shell.

Figure 2

(a) Crystal structure of K2NpO4 (K atoms in purple, O atoms in red, NpO6 octahedra in gray) showing the sheets of corner-sharing NpO6 octahedra in the (ab) plane. (b) NpO6 octahedron in K2NpO4 with the neptunyl type of coordination.

Comparison between the observed (Yobs, in red) and calculated (Ycalc, in black) X-ray diffraction patterns of K2NpO4 collected at room temperature (T = 295 ± 2 K). Yobs – Ycalc, in blue, is the difference between the experimental and calculated intensities. The Bragg reflection angular positions are marked in green. The inset shows an enlargement of the refinement in the angle range 2θ = 70–120°. Measurements were carried out with λ = Cu Kα1 radiation. (a) Crystal structure of K2NpO4 (K atoms in purple, O atoms in red, NpO6 octahedra in gray) showing the sheets of corner-sharing NpO6 octahedra in the (ab) plane. (b) NpO6 octahedron in K2NpO4 with the neptunyl type of coordination. Rwp = 13.5, Rexp = 5.37, χ2 = 6.29. N is the number of atoms in each coordination shell. The XANES spectrum of K2NpO4 collected at the Np-L3 edge is shown in Figure together with those of NpO2, Na3NpVO4, α-Na2NpVIO4, Na4NpVIO5, and Na5NpVIIO6 reference materials.[10] The valence states of the sodium neptunates were confirmed by 237Np Mössbauer spectroscopy from the values of their isomer shifts,[5−7] while the corresponding XANES spectra were reported in ref (10). The values of the measured inflection points and white lines are reported in Table . The investigated series covered a wide range of oxidation states (IV–VII) and a variety of local coordination geometries around the neptunium cation, i.e., neptunyl (Na3NpO4 and α-Na2NpO4), “reverse” neptunyl (Na4NpO5), and distorted NpO6 octahedra (Na5NpO6), which has allowed us to correlate the shape of the XANES spectra with the local structural environments,[10] as described later in this paper.
Figure 3

Normalized XANES spectrum of K2NpO4 (present work) together with those of NpO2, Na3NpO4, α-Na2NpO4, Na4NpO5, and Na5NpO6 reference materials.[10]

Table 3

Energies of the Inflection Points and White Lines of the Np-L3 XANES Spectraa

  white line (eV)
 
compoundinflection point (eV)  ref
K2NpO417614.5(5)17620.2(5)17631.5(5)this work
NpIVO217612.1(5)17618.3(5) (10)
Na3NpVO417613.4(5)17618.5(5) (10)
α-Na2NpVIO417614.2(5)17624.3(5) (10)
Na4NpVIO517614.1(5)17618.8(5)17625.6(5)(10)
Na5NpVIIO617615.1(5)17619.0(5)17626.9(5)(10)

The secondary white line, if present, is given in italics.

Normalized XANES spectrum of K2NpO4 (present work) together with those of NpO2, Na3NpO4, α-Na2NpO4, Na4NpO5, and Na5NpO6 reference materials.[10] The secondary white line, if present, is given in italics. The inflection point position of K2NpO4, corresponding to the absorption edge threshold E0 for the 2p → 6d transitions, is well aligned with those of α-Na2NpVIO4 and Na4NpVIO5 (Table ). These results confirm that neptunium is exclusively in the oxidation state VI in K2NpO4, corresponding to a [Rn]5f1 electronic configuration. The Np ion in this structure is therefore a Kramers ion with a 2F5/2 ground state manifold, and a 2F7/2 first excited state arising from spin–orbit coupling. Smith et al. reported a linear correlation of the absorption edge threshold E0 determined by XANES versus the Mössbauer isomer shift for the series of sodium neptunates.[10] The value for K2NpO4 fits very well with this trend (Figure ) when the isomer shift value determined by Nectoux et al. is used: i.e., δIS = −56.9(6) mm s–1 at 4.2 K relative to the standard NpAl2 absorber.[8] The linear variation between E0 and δIS can be understood from the fact that both quantities result from the Coulomb interaction with the surrounding electrons. The 5f shells produce a shielding effect on the electronic charge density of the s1/2 and p1/2 inner shells, which affects the isomer shift: δIS = α[Δρe(0)] (α being a calibration constant and Δρe(0) the difference in electronic charge density between the source material and the absorber at the nuclear origin). ρe(0) increases with the removal of 5f electrons. Moreover, the increase in formal valence state produces a decrease in Coulomb energy in the final state between the 5f and 6d electrons and the 2p3/2 core hole,[20−22] which leads to a shift to higher energy of the absorption edge threshold E0.
Figure 4

Absorption edge threshold E0 relative to NpO2 versus isomer shift measured by Mössbauer spectroscopy.

Absorption edge threshold E0 relative to NpO2 versus isomer shift measured by Mössbauer spectroscopy. In addition, the XANES spectrum of K2NpO4 shows the typical double-peaked white lines (WL) of Np(V), Np(VI), and Np(VII) compounds,[10,20,21] while the tetravalent NpIVO2 compound exhibits a single WL peak. The double peak consists of the main white line at 17620.2(5) eV and a shoulder and reduced peak amplitude about 15 eV above the Np edge. This feature has traditionally been attributed to localized multiple-scattering resonance of the neptunyl configuration. However, studies[10] on the sodium uranates and neptunates have shown that the correlation between the shape of the XANES spectra and the local coordination geometries is probably more intricate. The isostructural compounds α-Na2UVIO4 and α-Na2NpVIO4, presenting a neptunyl type of configuration, do not show the expected secondary shoulder and reduced peak amplitude, whereas Na4UVIO5, presenting a “reverse” neptunyl type of configuration, does.[10] Other factors could play a role, and effects of the degree of localization of the 5f electrons[10] and core-ionized final states with different 5f occupancies[20,21] have been suggested. The absorption edge threshold E0 is finally slightly higher (0.3 eV) for K2NpO4 than for α-Na2Np(VI)O4, which could be related to the neptunyl bond distances (Table ), degree of covalency, or (in other words) degree of localization of the 5f electrons in both compounds. The shorter the Np–O bonds, the more localized the 5f electrons, and the greater the Coulomb energy, making it easier to eject an electron from the 2p3/2 core–shell. However, it is not possible to conclude definitively, given the experimental uncertainties (0.5 eV) of the measurements at the Np-L3 edge, and this would require performing high-energy-resolution fluorescence-detected (HERFD) XANES measurements at the M4 edge.

Heat Capacity Measurements

The heat capacity data of K2NpO4 and K2UO4 measured at low temperatures in the absence of a magnetic field are shown in Figure and given in Tables and 6 of the Appendix. The two curves cross above T = 150 K, although one would expect them to become equal, corresponding to the same lattice contribution at high temperatures for the uranium and neptunium compounds. However, this discrepancy can be related on the one hand to the uncertainty on our experimental results, which increases toward high temperatures using the PPMS technique, and on the other hand to the fact that one compound was measured with Stycast and the other without. The uncertainty on the neptunium data corrected for the Stycast contribution is around 3% at room temperature, whereas that of the uranium data measured without Stycast is around 1%. The heat capacities reach values that are about 17–24 J K–1 mol–1 below the classical Dulong–Petit limit (Clat = 21R ≈ 174.6 J K–1 mol–1 for the seven atoms in the formula unit) as the temperature approaches 298.15 K.
Figure 5

Heat capacity of K2NpO4 (black ○) and K2UO4 (blue □) measured in zero magnetic field and the numerical fit to the neptunium (red line) and uranium (blue dotted line) data.

Table 5

Experimental Heat Capacity Data for K2NpO4

T (K)Cp,m (J K–1 mol–1)T (K)Cp,m (J K–1 mol–1)T (K)Cp,m (J K–1 mol–1)T (K)Cp,m (J K–1 mol–1)
298.43150.5485.0278.55424.4215.8446.480.34949
294.03150.8683.9977.75523.8514.7566.370.33499
289.93150.3382.9676.91123.3613.9006.280.32159
285.82149.6981.9376.12922.8412.9986.180.30762
281.73149.5880.8975.29322.3112.0916.080.29390
277.63149.8279.8674.40221.7811.2825.990.28239
273.52149.7478.8373.56521.2710.5625.890.27128
269.43149.5177.8072.67720.759.88375.800.26038
265.33149.0876.7671.78220.239.23235.710.24960
261.22148.5575.7270.85920.209.17665.620.23952
257.14148.0274.6669.96519.878.79475.540.22983
253.02147.7473.6369.06719.618.47945.450.22093
248.91147.3472.5868.16119.338.14745.370.21260
244.82146.5271.5567.25319.027.79215.280.20444
240.71145.8070.5266.32618.637.38315.200.19678
236.60144.7669.4665.34218.407.14135.120.18957
232.49143.7268.4564.35118.056.79135.050.18253
228.38142.9467.3763.33617.836.55884.970.17529
224.26141.9266.3662.32517.506.24514.890.16922
298.44150.3165.3361.28317.266.00074.810.16271
294.01150.4664.2960.23216.985.74534.740.15676
289.93149.8963.2859.19116.715.50904.670.15113
285.82149.4362.2158.12816.465.28714.590.14569
281.73149.1761.1957.07716.195.05704.530.14069
277.62149.4560.1456.01315.934.84134.460.13668
273.52149.5959.1154.95115.694.64264.400.13278
269.43149.2158.0653.88615.444.43864.330.12729
265.34148.9657.0452.79715.204.24454.270.12352
261.22148.3756.0151.69114.964.06314.210.11882
257.14147.8654.9850.56514.733.88844.140.11501
253.02147.6853.9349.40914.493.71474.080.11167
248.92147.1552.8948.23714.263.54664.020.10681
244.82146.4151.8747.08614.043.39253.960.10417
240.71145.6350.8245.96613.823.24453.900.10116
236.61144.6849.7844.77113.603.10123.849.8110 × 10–2
232.49143.6148.7543.56613.392.96533.789.5240 × 10–2
228.38142.9247.7442.34713.182.83243.739.2290 × 10–2
224.29141.8946.7041.10112.972.70423.689.0240 × 10–2
220.16140.7545.6639.88912.772.58223.618.7210 × 10–2
216.06139.8945.6639.88012.572.46843.568.5010 × 10–2
211.94138.8045.1239.23412.372.35543.518.3120 × 10–2
207.84137.7244.6038.61612.182.25143.468.1080 × 10–2
203.72136.8544.0838.03111.992.14803.417.9860 × 10–2
199.59135.6543.5737.42911.802.04713.377.8210 × 10–2
195.49134.4143.0536.82111.611.95343.327.6230 × 10–2
191.37132.9842.5336.20911.431.86093.277.4610 × 10–2
187.26131.5842.0135.59611.241.77613.237.3660 × 10–2
183.14130.3841.5034.98011.071.69783.187.1800 × 10–2
179.02129.0840.9634.33810.891.62203.137.0580 × 10–2
174.90127.6440.3433.62310.721.54773.086.8430 × 10–2
170.78126.1539.8533.08210.561.47753.046.7060 × 10–2
166.67124.6739.3232.47510.391.40863.006.5610 × 10–2
162.55123.1438.8031.87510.231.34482.956.4510 × 10–2
158.43121.5738.2831.28410.071.28502.916.3420 × 10–2
154.30120.0137.7730.6789.911.22732.886.2390 × 10–2
150.18118.3537.2730.1039.761.17172.846.1410 × 10–2
146.05116.7336.7429.4929.611.11752.806.0530 × 10–2
141.92114.8536.2328.9019.461.06652.765.9840 × 10–2
137.79112.9735.7028.3009.311.01642.735.8780 × 10–2
133.66110.9435.1927.7099.160.970512.695.8210 × 10–2
129.51108.5234.6727.1259.020.926992.655.7300 × 10–2
125.39106.4734.1626.5548.880.884532.625.6670 × 10–2
121.26104.2333.6425.9778.740.844642.585.5870 × 10–2
117.14101.8633.1225.3998.610.806412.555.4840 × 10–2
113.0099.34232.6124.8348.470.769522.525.4310 × 10–2
108.8596.70532.1024.2508.340.733722.495.3670 × 10–2
104.7393.92531.5823.6828.210.700412.465.2780 × 10–2
100.5990.93631.0723.1198.080.668012.435.2170 × 10–2
96.4487.77430.5522.5747.960.637532.405.1490 × 10–2
96.4987.82630.0522.0497.830.606852.375.0650 × 10–2
95.3586.88429.5621.5687.710.579812.345.0040 × 10–2
94.3186.10829.0321.0687.590.553022.314.9240 × 10–2
93.2885.26328.5120.6247.480.527772.284.8980 × 10–2
92.2484.46728.0020.2277.360.504072.264.8450 × 10–2
91.2283.65827.4819.9087.250.480992.234.7590 × 10–2
90.1982.86726.9519.7557.130.459422.214.7150 × 10–2
89.1682.00326.4719.8276.930.422532.184.6610 × 10–2
88.1281.11525.9619.7386.780.397662.164.6260 × 10–2
87.0880.20425.4618.4596.680.380072.134.5250 × 10–2
86.0579.39524.9517.0546.580.36403  
Table 6

Experimental Heat Capacity Data for K2UO4

T (K)Cp,m (J K–1 mol–1)T (K)Cp,m (J K–1 mol–1)T (K)Cp,m (J K–1 mol–1)T (K)Cp,m (J K–1 mol–1)
312.40161.6087.1282.81027.3815.2987.480.39842
312.39160.5887.1282.83226.8714.6657.480.39873
312.43160.2483.0679.36626.8814.7087.490.39950
308.36159.0883.0879.37126.8814.7107.310.36697
308.60159.4583.0779.38426.3614.1137.310.36579
308.62159.1879.0175.67626.3714.1247.310.36601
304.47158.2079.0375.69126.3614.1187.130.33632
304.70158.3979.0375.66625.8513.5457.140.33672
304.69158.1274.9671.82625.8613.5527.140.33674
300.55157.4274.9871.83825.8613.5386.990.31321
300.75157.5574.9771.82025.3512.9676.990.31255
300.73157.4570.9267.79525.3612.9936.990.31434
296.58156.8070.9367.82925.3512.9886.810.28615
296.75157.0770.9367.79524.8412.4256.820.28738
296.76156.8766.8763.59624.8512.4326.820.28696
292.59156.1466.8963.61124.8512.4316.650.26296
292.77156.3566.8863.57024.3311.8976.660.26242
292.78156.3362.8259.11324.3411.8836.660.26271
288.60155.0962.8459.11324.3411.8756.500.24180
288.78155.4362.8459.10023.8311.3646.500.24290
288.76155.3058.7854.55223.8411.3336.500.24231
284.60154.4958.7954.56823.8311.3276.340.22326
284.76154.6458.7954.56323.3210.7866.350.22277
284.75154.6054.7449.80123.3310.7986.350.22412
280.59154.0154.7549.81623.3310.7896.200.20715
280.75154.3554.7449.79322.8110.2946.200.20732
280.74154.1550.6944.91722.8210.2756.200.20594
276.58153.7850.7044.92722.8210.2626.050.18998
276.73153.8750.6944.91022.319.75236.050.19010
276.73153.8150.7144.95522.319.73816.060.19027
272.57153.1550.6944.92222.319.74625.910.17522
272.73153.4650.6944.89821.809.23195.910.17396
272.71153.2950.1644.24921.809.23385.910.17499
268.56152.7350.1944.28121.809.23295.770.16011
268.70152.8350.1944.27921.308.72705.770.16012
268.70152.8349.6643.61721.308.74105.780.16111
264.55152.1049.6843.65521.308.73815.640.14760
264.67152.3149.6843.65720.798.25525.640.14831
264.68152.2949.1542.98720.798.25905.640.14809
260.53151.1749.1843.03120.798.25725.500.13636
260.65151.4449.1743.03420.287.78235.510.13711
260.65151.4248.6542.34820.297.79525.510.13768
256.51150.5548.6742.38620.287.78255.370.12648
256.63150.7048.6742.39520.277.76595.380.12664
256.64150.6748.1441.72320.287.78665.380.12708
252.49150.0148.1741.76820.287.79185.250.11747
252.62150.1848.1641.76219.817.35405.250.11869
252.62150.1047.6341.07719.827.39275.250.11884
248.48149.3747.6641.12619.807.34815.130.10952
248.61149.5147.6641.13219.346.93565.130.10936
248.59149.5047.1340.44519.356.95825.130.11049
244.46148.5247.1540.48619.346.93585.010.10157
244.57148.7147.1540.49318.886.53735.019.9880 × 10–2
244.57148.8346.6239.81018.896.54275.019.9880 × 10–2
240.45147.7846.6439.85718.896.54364.899.2890 × 10–2
240.54147.8446.6439.84018.456.15794.899.2690 × 10–2
240.54147.8946.1139.16218.456.17554.899.2930 × 10–2
236.41146.8546.1439.19618.446.16734.778.5980 × 10–2
236.51147.0246.1439.19518.005.80384.778.6130 × 10–2
236.52146.9145.6138.52818.025.81474.778.6140 × 10–2
232.38145.8445.6338.55118.025.81414.667.9830 × 10–2
232.49145.9645.6338.55517.595.46224.667.9230 × 10–2
232.48146.0245.1037.87017.605.47854.667.9820 × 10–2
228.37145.0845.1237.91217.595.47394.557.3160 × 10–2
228.46145.1045.1237.90017.185.15044.557.5280 × 10–2
228.46145.0544.5937.22417.195.15504.557.4780 × 10–2
224.34144.2444.6237.25617.185.15314.436.9070 × 10–2
224.43144.3744.6237.25316.784.84084.446.8680 × 10–2
224.45144.3444.0936.55616.784.85194.446.8210 × 10–2
220.32143.3044.1136.59916.784.84674.336.4690 × 10–2
220.41143.4144.1136.59316.384.55974.346.3390 × 10–2
220.41143.3143.5835.90316.394.56034.336.5490 × 10–2
216.30142.3343.6035.94416.384.55524.235.9750 × 10–2
216.38142.3143.6035.93715.994.27254.246.0840 × 10–2
216.38142.3943.0735.25716.014.28164.235.9510 × 10–2
212.25141.2443.1035.29816.004.27754.135.5180 × 10–2
212.35141.4043.0935.28315.624.01264.135.5460 × 10–2
212.35141.4142.5734.59715.634.01634.135.5940 × 10–2
208.24140.1542.5934.63215.624.01554.045.2470 × 10–2
208.31140.2242.5934.62615.253.76464.045.1320 × 10–2
208.31140.2442.0633.93915.263.77454.045.1380 × 10–2
204.21139.0742.0833.96715.263.77163.944.7470 × 10–2
204.28139.2242.0833.97314.893.53003.944.7740 × 10–2
204.28139.2041.5533.27214.913.53493.944.7650 × 10–2
200.18138.0041.5733.31114.903.53743.854.4080 × 10–2
200.25138.0641.5733.30114.543.30813.854.4050 × 10–2
200.26138.0441.0532.61914.553.31173.854.4260 × 10–2
196.14136.8141.0732.66014.553.31413.764.1200 × 10–2
196.22136.9241.0632.64414.203.09473.764.0950 × 10–2
196.22136.9440.5431.95714.213.10073.764.0910 × 10–2
192.11135.6840.5631.98814.213.09873.673.8110 × 10–2
192.18135.7740.5631.99413.862.89533.673.8120 × 10–2
192.18135.7140.0331.30213.882.90213.673.7950 × 10–2
188.08134.4740.0531.33313.882.90383.583.5360 × 10–2
188.15134.5240.0531.32713.542.71243.583.5480 × 10–2
188.15134.5339.5330.64813.552.71093.593.4990 × 10–2
184.05133.2939.5530.67513.552.71553.503.2930 × 10–2
184.12133.2639.5430.67013.222.53163.503.3200 × 10–2
184.12133.2639.0229.98713.232.53473.503.3020 × 10–2
180.04132.0139.0430.02113.232.53533.423.0580 × 10–2
180.08132.1339.0430.02412.912.35723.423.0950 × 10–2
180.09132.0438.5129.34012.922.36443.423.1160 × 10–2
176.01130.6538.5329.37412.932.36763.342.8860 × 10–2
176.07130.7038.5329.37212.612.20343.342.8800 × 10–2
176.06130.7138.0128.67212.622.20603.342.8840 × 10–2
171.98129.2438.0328.71812.622.20453.262.6860 × 10–2
172.03129.2838.0228.70412.322.05493.262.6890 × 10–2
172.03129.3637.5028.02912.332.05613.262.6860 × 10–2
167.95127.9437.5228.06212.332.06113.182.4880 × 10–2
167.99127.9537.5228.05312.031.91463.182.4850 × 10–2
167.98127.9736.9927.37412.031.91763.192.5250 × 10–2
163.91126.5137.0127.39612.031.91713.112.3250 × 10–2
163.95126.5137.0127.39811.741.78033.112.3450 × 10–2
163.95126.5136.4926.70811.751.78353.112.3410 × 10–2
159.88125.0136.5126.73611.761.78713.042.1950 × 10–2
159.91125.0436.5126.72311.471.65523.042.1950 × 10–2
159.91124.9835.9826.04311.481.65783.042.2000 × 10–2
155.84123.3636.0026.08311.481.65792.972.0570 × 10–2
155.86123.4536.0026.07311.201.54022.972.0520 × 10–2
155.86123.4135.4725.37311.211.54282.972.0350 × 10–2
151.80121.7535.4925.42811.211.54402.901.9310 × 10–2
151.82121.6935.4925.40510.941.43022.901.9280 × 10–2
151.82121.7334.9724.74110.951.43062.901.9470 × 10–2
147.77120.0934.9924.77110.951.43222.831.5950 × 10–2
147.79120.0834.9824.75810.681.32592.841.6010 × 10–2
147.78120.1034.4624.08310.691.33002.841.6110 × 10–2
143.72118.3634.4824.12310.691.33152.771.5000 × 10–2
143.74118.3434.4824.10310.441.23102.771.4920 × 10–2
143.74118.3433.9523.43910.441.23132.771.4920 × 10–2
139.68116.3833.9823.46210.441.23112.701.4020 × 10–2
139.70116.4033.9723.45810.191.13842.701.3910 × 10–2
139.70116.3433.4522.78010.201.14082.701.3920 × 10–2
135.65114.3433.4722.82110.201.14192.641.3010 × 10–2
135.66114.3533.4722.8029.961.05512.641.2920 × 10–2
135.66114.3132.9522.1529.961.05612.641.2950 × 10–2
131.61112.2832.9622.1609.961.05562.571.2100 × 10–2
131.62112.2632.9622.1719.720.974012.571.2060 × 10–2
131.62112.2432.4421.5049.730.976472.571.1990 × 10–2
127.57110.1032.4621.5359.730.976722.521.1270 × 10–2
127.57110.1032.4521.5289.490.900852.521.1280 × 10–2
127.57110.0731.9420.8709.500.900272.521.1220 × 10–2
123.53107.8931.9520.8899.500.901002.461.0530 × 10–2
123.54107.8431.9520.8899.260.830452.461.0520 × 10–2
123.54107.8731.4320.2349.280.831692.451.0470 × 10–2
119.50105.4531.4420.2559.280.832792.409.8700 × 10–3
119.49105.4431.4420.2439.040.767992.409.7700 × 10–3
119.49105.3930.9219.5959.050.768062.409.8000 × 10–3
115.45103.0030.9419.6089.050.769232.349.2100 × 10–3
115.45102.9830.9419.6148.830.706912.349.1500 × 10–3
115.45103.0430.4218.9578.840.707622.349.1500 × 10–3
111.41100.4830.4318.9778.840.708422.298.5700 × 10–3
111.39100.4630.4318.9808.630.653152.298.5500 × 10–3
111.40100.5229.9118.3418.630.653402.298.5400 × 10–3
107.3597.85629.9218.3518.630.654122.247.9200 × 10–3
107.3597.83929.9218.3418.420.601712.247.9300 × 10–3
107.3497.80529.3917.7168.430.600402.237.9100 × 10–3
103.3095.05329.4217.7368.430.600892.187.4100 × 10–3
103.3095.04729.4117.7228.230.554102.187.3900 × 10–3
103.3095.01328.8917.0958.230.553962.187.3700 × 10–3
99.2592.19328.9117.1208.230.554802.146.8700 × 10–3
99.2592.17228.9017.1108.030.512322.146.8600 × 10–3
99.2592.19228.3916.5048.040.511772.146.8500 × 10–3
95.2189.27228.3916.4978.040.511782.096.3900 × 10–3
95.2089.27328.4016.5077.840.470832.096.3700 × 10–3
95.2189.21627.8915.9017.850.470062.096.3500 × 10–3
91.1686.17927.8915.9037.850.470402.035.9000 × 10–3
91.1586.10427.8915.9167.660.432542.035.8700 × 10–3
91.1686.11227.3815.2857.670.433282.045.9200 × 10–3
87.1182.90127.3815.3047.670.43355  
Heat capacity of K2NpO4 (black ○) and K2UO4 (blue □) measured in zero magnetic field and the numerical fit to the neptunium (red line) and uranium (blue dotted line) data. The collected data for K2NpO4 show a small anomaly at T = 25.9 K, which is almost unaffected by the application of a 9 T magnetic field apart from a small decrease in the amplitude. This feature could be interpreted at first as an indication of the presence of NpO2 impurity within the investigated material. Indeed, neptunium dioxide shows a sharp λ anomaly at T = 25.7 K[23,24] due to rank 5 triacontadipolar order as described in the studies of Santini et al.,[25] with a similar behavior upon application of a magnetic field. However, the X-ray diffraction data did not reveal any secondary NpO2 phase. Moreover, the shape of the anomaly in K2NpO4 does not match that of NpO2, although the critical temperatures are very close. The anomaly is very symmetrical in K2NpO4, in contrast with NpO2, showing an asymmetrical profile. On the basis of its amplitude, the amount of NpO2 impurity would correspond to 26.9 ± 1.0%, which should be detected easily by the X-rays. We conclude that the anomaly is an intrinsic property of K2NpO4. The corresponding magnetic contribution was derived as Smag = 3.1 ± 0.1 J K–1 mol–1 after subtraction of the lattice heat capacity contribution (Figure ). The latter was approximated with the heat capacity of K2UO4 (which has electronic configuration [Rn]5f0), as the two compounds are isostructural and have very similar atomic masses. The derived magnetic entropy value represents about 53.8% of the expected order–disorder entropy for such a Kramers system (Smag = Rln2). It is worth pointing out that a low magnetic entropy, i.e. 0.19Rln2, has also been reported for α-Na2NpO4.[7]
Figure 7

Electronic contribution to the heat capacity in K2NpO4 obtained by subtracting the data for K2UO4.

Interestingly, no anomaly was observed around 19.5(5) K, as could be expected from the Mössbauer results of Nectoux et al.[8] An X-ray diffraction pattern collected after the low-temperature heat capacity measurement moreover confirmed that the sample had retained its integrity during the experiment. Since the magnetic susceptibility measurements of the authors also did not show any anomaly around 20 K,[8] the existence of a first-order magnetic phase transition at the latter temperature is unlikely. To explain the origin of the magnetic hyperfine splitting reported below 19.5(5) K, we could suggest the occurrence of a slow electron spin relaxation phenomenon in this paramagnetic system.[26] However, this is doubtful, as it would require a sudden collapse of the relaxation time at the critical temperature. The cell parameters reported by[8] for K2NpO4 (a = 4.26 Å and c = 13.01 Å) are lower than those found in this study. A contamination of their sample with a magnetic impurity is possible although unlikely, as they reported a single-phase material, but they give very little detail on phase preparation and purity. The magnetic hyperfine splitting effect observed by the authors probably corresponds to the anomaly observed herein at 25.9 K, with a somewhat lower critical temperature. It should be pointed out that differences in critical temperatures of about 3–8 K have been reported in the literature between Mössbauer and magnetic susceptibility results of the uraniumneptunium mixed oxides U1–NpO2.[27] For the magnetic susceptibilty results of Nectoux et al., a clear deviation from the Curie–Weiss law is observed below about 40 K, which could suggest ferromagnetic ordering below the latter temperature. The hypothesis of a ferromagnetic transition is moreover in good agreement with the low-temperature heat capacity data, showing a slight decrease of the anomaly at T = 25.9 K upon application of a magnetic field. The negative value of the Curie constant, i.e., ΘP = −150 K, derived from the Curie–Weiss analysis of the data[8] is rather surprising, however. It suggests a more complex order, possibly with a canting of the ferromagnetically coupled moments or with strong antiferromagnetic interactions. In the present work, the thermodynamic functions of K2NpO4 and K2UO4 were derived at 298.15 K by fitting the experimental data to theoretical functions below T = 8.0 K and T = 20.0 K,[28] respectively, and a combination of Debye and Einstein heat capacity functions[29−31] at T = 7.8–298.4 K and at T = 20.0–312.4 K, respectively. The fitted data are shown with solid and dotted lines in Figures and 6. The heat capacity values at 298.15 K were obtained by interpolation, yielding Cp,mo(K2NpO4, cr, 298.15 K) = 152.7 ± 4.5 J K–1 mol–1 and Cp,mo(K2UO4, cr, 298.15 K) = 156.5 ± 1.6 J K–1 mol–1 (in both cases, the quoted uncertainty corresponds to the standard uncertainty). The experimental standard entropies at 298.15 K were determined by numerical integration of Cp,m/T = f(T) using the aforementioned fitted functions and including the magnetic entropy contribution, yielding Smo(K2NpO4, cr, 298.15 K) = 209.3 ± 4.9 J K–1 mol–1 and Smo(K2UO4, cr, 298.15 K) = 210.1 ± 2.7 J K–1 mol–1, respectively. The values obtained for K2NpO4 are slightly lower than that of K2UO4, whereas the inverse behavior would be expected. However, this is due to the uncertainty introduced by the use of Stycast as mentioned before and the crossing of the two curves. When adding the derived magnetic entropy to the lattice contribution of K2UO4, one derives 213.2 J K–1 mol–1 for the standard entropy of K2NpO4, which remains within the uncertainty of the present measurement.
Figure 6

Cp/T for K2NpO4 (black ○) and K2UO4 (blue □) measured in zero magnetic field and the numerical fit to the neptunium (red line) and uranium (blue dotted line) data.

Cp/T for K2NpO4 (black ○) and K2UO4 (blue □) measured in zero magnetic field and the numerical fit to the neptunium (red line) and uranium (blue dotted line) data.

Fitting of the Lattice Contribution above T = 8.0 K (K2NpO4) and T = 20.0 K (K2UO4)

At very low temperatures where the thermal expansion is negligible, the heat capacity at constant pressure can be approximated to the heat capacity at constant volume Cp,m ≈ CV,m, which comprises lattice vibrations, electronic, and magnetic contributions[32] The lattice contribution dominates at temperatures above about T = 8–20 K and can be modeled using a combination of Debye and Einstein functions, as shown in eq . Two Einstein functions were used in this work to fit the data. Fitting with a single Einstein function was attempted but could not reproduce accurately the high-temperature region:where R is the universal gas constant equal to 8.3144621 J K–1 mol–1, D(Θ), E(Θ), and E(Θ) are the Debye and Einstein functions, respectively, as written in eqs and 3. ΘD, ΘE1, and ΘE2 are the characteristic Debye and Einstein temperatures. nD, nE1, and nE2 are adjustable parameters, whose sum nD + nE1 + nE2 should be approximately equal to the number of atoms in the formula unit (i.e., 7 in this case). The fitted parameters are listed in Table . The sum nD + nE1 + nE2 is very close to 7.
Table 4

Summary of Fitting Parameters of the Heat Capacities of K2NpO4 and K2UO4

Debye and Einstein fit
harmonic lattice model
    
K2NpO4
temp range/K7.71–298.4temp range/K2.1–8.0
nD/mol2.3637δ/mJ mol–1 K–122.25
ΘD/K154.41B3/mJ mol–1 K–4–5.00553 × 10–1
nE1/mol1.9806B5/mJ mol–1 K–66.48526 × 10–2
ΘE1/K588.19B7/mJ mol–1 K–8–1.13475 × 10–3
nE2/mol2.5292B9/mJ mol–1 K–107.32029 × 10–6
θE2/K287.56  
nD + nE1 + nE2 mol6.87  
K2UO4
temp range/K19.8–312.4temp range/K2.0–20.3
nD/mol2.0522δ/mJ mol–1 K–1 
ΘD/K157.08B3/mJ mol–1 K–46.43253 × 10–1
nE1/mol2.8798B5/mJ mol–1 K–67.77235 × 10–3
ΘE1/K256.28B7/mJ mol–1 K–8–4.50504 × 10–5
nE2/mol2.1601B9/mJ mol–1 K–101.03519 × 10–7
ΘE2/K610.54B11/mJ mol–1 K–12–8.70422 × 10–11
nD + nE1 + nE2/mol7.09  

Fitting below T = 8.0 K (K2NpO4) and T = 20.0 K (K2UO4)

At very low temperatures (T < 20 K), the phonon contribution is well-represented using a harmonic lattice model,[28] as expressed by the polynomial function (, where the number of required terms augments the high-temperature limit of the fit:The electronic contribution of the conduction electrons at the Fermi surface are represented with the linear term γT.[33] For insulating materials such as K2NpO4 and K2UO4, the electronic specific heat is 0. However, a linear term was reported in materials such as α-FeOOH,[28] Fe3(P2O7)2,[34] and Sr2TiSi2O8,[35] which was related to departure from stoichiometry, oxygen vacancies, or defects within the material.[28] The heat capacity of K2NpO4 was fitted with the harmonic model using four terms over the temperature range T = 2.1–8.0 K. That of K2UO4 was fitted with five terms over the temperature range T = 2.0–20.3 K. The corresponding coefficients are given in Table . In addition, the use of a linear δT term appeared necessary to describe the experimental curve of K2NpO4. More recently, the occurrence of such a linear term was also reported in Na4NpO5,[36] which was related to the presence of defects within the material and an asymmetric peak profile shape in opposite directions for successive hkl reflections clearly visible on the X-ray diffraction pattern. The X-ray diffraction data of K2NpO4 do not show such features, however. Self-heating effects coming from the radioactive decay of 237Np were considered but appeared negligible. Moreover, departure from stoichiometry is unlikely according to the present Np-L3 XANES results and Mössbauer data of ref (8). Hence, the physical origin of this feature remains unclear. The appearance of a nuclear Schottky effect arising from the magnetic hyperfine splitting interaction between the unpaired 5f electron and the magnetic moment at the Np nucleus (I = 5/2) was suggested for Na2NpO4, as the corresponding data showed a reincrease below 3.7 K.[37] K2NpO4 might show similar behavior (Figure ), but we cannot conclude in the absence of data below 2.0 K, which would require complementary measurements using a 3He refrigerator. Electronic contribution to the heat capacity in K2NpO4 obtained by subtracting the data for K2UO4.

Conclusion

A Rietveld refinement of the crystal structure of K2NpO4, tetragonal in space group I4/mmm, is reported for the first time in the present work. The refined cell parameters and bond lengths are in good agreement with the trend of decreasing ionic radii along the actinide series. XANES data have also been collected at the Np-L3 edge, which have confirmed the hexavalent state of neptunium in this compound and therefore the assigned stoichiometry. The measured absorption edge threshold E0 fits very well the linear correlation observed for the sodium neptunates between E0 and the isomer shift value δIS measured by Mössbauer spectroscopy. Moreover, double-peak white lines have been observed for K2NpO4, which are usually attributed to multiple scattering resonances of the actinyl compounds, but the interpretation could be more intricate. Electronic density calculations are needed to obtain more insight into those complex features. Low-temperature heat capacity data have been collected in the temperature range T = 2.1–298.4 K for K2NpO4 and T = 2.0–312.4 K for K2UO4, and the standard entropy and heat capacity of both compounds have been derived at 298.15 K. The latter data have revealed the presence of an anomaly at 25.9 K with an associated magnetic entropy Smag = 3.1 ± 0.1 J K–1 mol –1, which most probably corresponds to the magnetic hyperfine splitting event observed in the literature by Mössbauer spectroscopy at a slightly lower temperature: i.e., T = 19.5(5) K.[8] Both the present low-temperature heat capacity data and the magnetic susceptibility measurements of Nectoux et al.[8] are consistent with the hypothesis of a ferromagnetic ordering transition around T = 25.9 K. Complementary studies involving repeated Mössbauer spectroscopy and magnetic susceptibility measurements, as well as neutron diffraction measurements on a well-characterized material, would allow confirmation of those results. Finally, the amplitude of the anomaly at 25.9 K is smaller than expected for this Kramers system (Smag = R ln 2), but similar results have also been reported for α-Na2NpO4. The low values of the ordered moment derived from the Mössbauer data (∼0.6 μB), of the paramagnetic effective moment derived from the magnetic susceptibility data (μeff = 1.37 μB), and of the magnetic entropy (Smag = 0.538R ln 2), are not unusual for 5f1 systems. Further investigations involving spectroscopy measurements at low energy and theoretical calculations are clearly required to get further insight into the Np(VI) crystal-field ground state and magnetic behavior of the alkali and alkaline-earth neptunates.
  9 in total

1.  Electronic structure of actinide compounds from LIII-edge x-ray absorption.

Authors: 
Journal:  Phys Rev Lett       Date:  1989-12-11       Impact factor: 9.161

2.  ATHENA, ARTEMIS, HEPHAESTUS: data analysis for X-ray absorption spectroscopy using IFEFFIT.

Authors:  B Ravel; M Newville
Journal:  J Synchrotron Radiat       Date:  2005-06-15       Impact factor: 2.616

3.  Hidden order and low-energy excitations in NpO2.

Authors:  P Santini; S Carretta; N Magnani; G Amoretti; R Caciuffo
Journal:  Phys Rev Lett       Date:  2006-11-14       Impact factor: 9.161

4.  X-ray Diffraction, Mössbauer Spectroscopy, Magnetic Susceptibility, and Specific Heat Investigations of Na4NpO5 and Na5NpO6.

Authors:  Anna L Smith; Amir Hen; Philippe E Raison; Eric Colineau; Jean-Christophe Griveau; Nicola Magnani; Jean-Pierre Sanchez; Rudy J M Konings; Roberto Caciuffo; Anthony K Cheetham
Journal:  Inorg Chem       Date:  2015-04-10       Impact factor: 5.165

5.  A new look at the structural properties of trisodium uranate Na3UO4.

Authors:  Anna L Smith; Philippe E Raison; Laura Martel; Damien Prieur; Thibault Charpentier; Gilles Wallez; Emmanuelle Suard; Andreas C Scheinost; Christoph Hennig; Philippe Martin; Kristina O Kvashnina; Anthony K Cheetham; Rudy J M Konings
Journal:  Inorg Chem       Date:  2015-03-23       Impact factor: 5.165

6.  Structural investigation of Na3NpO4 and Na3PuO4 using X-ray diffraction and (237)Np Mössbauer spectroscopy.

Authors:  A L Smith; P E Raison; A Hen; D Bykov; E Colineau; J-P Sanchez; R J M Konings; A K Cheetham
Journal:  Dalton Trans       Date:  2015-09-15       Impact factor: 4.390

7.  Crystal-Field and Covalency Effects in Uranates: An X-ray Spectroscopic Study.

Authors:  Sergei M Butorin; Kristina O Kvashnina; Anna L Smith; Karin Popa; Philippe M Martin
Journal:  Chemistry       Date:  2016-06-03       Impact factor: 5.236

8.  Structural Properties and Charge Distribution of the Sodium Uranium, Neptunium, and Plutonium Ternary Oxides: A Combined X-ray Diffraction and XANES Study.

Authors:  Anna L Smith; Philippe Martin; Damien Prieur; Andreas C Scheinost; Philippe E Raison; Anthony K Cheetham; Rudy J M Konings
Journal:  Inorg Chem       Date:  2016-02-02       Impact factor: 5.165

9.  Mössbauer spectroscopy, magnetization, magnetic susceptibility, and low temperature heat capacity of α-Na₂NpO₄.

Authors:  Anna L Smith; Amir Hen; Nicola Magnani; Jean-Pierre Sanchez; Eric Colineau; Jean-Christophe Griveau; Philippe E Raison; Roberto Caciuffo; Rudy J M Konings; Anthony K Cheetham
Journal:  J Phys Condens Matter       Date:  2016-01-29       Impact factor: 2.333

  9 in total
  1 in total

1.  Lanthanide-Aromatic Iminodiacetate Frameworks with Helical Tubes: Structure, Properties, and Low-Temperature Heat Capacity.

Authors:  Ming-Li Liu; Quan Shi; Lei-Fang Liu; Wen-Bo Li
Journal:  ACS Omega       Date:  2021-04-12
  1 in total

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