Alessia
Provino
*abc,
Volodymyr
Smetana
ad,
Durga
Paudyal
a,
Karl A.
Gschneidner
Jr.
ad,
Anja-Verena
Mudring
ad,
Vitalij K.
Pecharsky
ad,
Pietro
Manfrinetti
abc and
Marina
Putti
ce
aThe Ames Laboratory, U.S. Department of Energy, Division of Materials Sciences and Engineering, Iowa State University, Ames, IA 50011-3020, USA. E-mail: alessia.provino@spin.cnr.it
bDepartment of Chemistry, University of Genova, Via Dodecaneso 31, 16146 Genova, Italy
cInstitute SPIN-CNR, Corso Perrone 24, 16152 Genoa, Italy
dDepartment of Materials Science and Engineering, Iowa State University, Ames, IA 50011-2300, USA
eDepartment of Physics, University of Genova, Via Dodecaneso 33, 16146 Genova, Italy
First published on 26th May 2016
The crystal structure, composition and physical properties of Gd3Ni2, which was earlier reported to exist in the Gd–Ni system without any details of its structure and properties, have been determined. This rare earth binary compound is a high-temperature phase: it forms via a peritectic reaction at 988 K (715 °C) and decomposes below ≈923 K (650 °C). The compound can be retained at room temperature as a metastable phase by quenching after high temperature annealing. Gd3Ni2 crystallizes in the monoclinic Dy3Ni2 structure type [mS20, C2/m (No. 12), Z = 4; with lattice parameters a = 13.418(3) Å, b = 3.720(1) Å, c = 9.640(2) Å, β = 106.250(3)°]. Ni can be substituted by Co up to 50% (i.e. up to and including Gd3CoNi) with no change in the structural prototype; the substitution of Co for Ni stabilizes the R3CoxNi2−x phases down to room temperature. The crystal structure, magnetic properties and magnetocaloric effect (MCE) have been investigated for both Gd3Ni2 and the related Gd3CoxNi2−x solid solution alloys (0 ≤ x ≤ 1). The crystal structure of the Gd3CoNi is a ternary ordered derivative of the monoclinic Dy3Ni2-type, where Co fully occupies only one of the two 4i Wyckoff sites available for the transition metal. To the best of our knowledge, this is the first example of an intermetallic phase showing ordered site occupations by the chemically quite similar elements Co and Ni. All compounds show long range ferromagnetic ordering, with TC progressively increasing from 147 K (for Gd3Ni2) to 176 K (for Gd3CoNi) as a cubic function of the Co content. Evidence of Co contributing to the magnetic interactions in these compounds has been found. First-principles total energy calculations predicted the ordered occupation of Co and Ni at the crystallographic sites of Gd3CoNi, which was later confirmed by single crystal X-ray diffraction. The increased conduction electronic state (3d) exchange splitting at the Fermi level supports the experimentally observed enhanced Curie temperature in Gd3CoNi compared to Gd3Ni2.
Despite a large number of known binary R–M compounds, there remain quite a few binary systems with reported but not fully investigated compounds. To mention some, ‘Nd2Co1.7’, ‘Gd3Ni2’, ‘Lu2Pd5’, ‘R2Pd3’, and ‘RPd2’ (R = rare earth)4–6 remain listed with uncertain compositions and unknown crystal structures. In the Gd–Ni binary system, a total of nine compounds have been reported to exist: Gd2Ni17, GdNi5, GdNi4, Gd2Ni7 (high- and low-temperature polymorphs), GdNi3, GdNi2, GdNi, Gd3Ni2 and Gd3Ni.4–7 The crystal structure has been determined for all of them except for ‘GdNi4’ and ‘Gd3Ni2’. The ‘Gd3Ni2’ phase was reported to form by a peritectic reaction at 690 °C with no additional structural details; a tetragonal cell with lattice parameters a = 7.28 Å and c = 8.61 Å has been proposed for this compound.8 However, more recent work indicated that ‘GdNi4’ and ‘Gd3Ni2’ do not exist,9 in apparent agreement with an earlier paper on this system.7 However, stoichiometric phases of composition R3Ni2 have been detected for R = Tb, Dy, Ho, Er, and Y; all of them form by a peritectic reaction (liquid + RNi). Tb3Ni2 and Dy3Ni2 are known to crystallize in the monoclinic Dy3Ni2-type [Pearson symbol mS20, space group C2/m (No. 12), Z = 4],10 while Er3Ni2 and Y3Ni2 crystallize in their own prototypes: the hexagonal Er3Ni2 [hR45, R (No. 148), Z = 9],11 and tetragonal Y3Ni2 [tP80, P41212 (No. 92), Z = 16],12 respectively. Ho3Ni2 is reported to be dimorphic, adopting the hexagonal Er3Ni2-type [the high-temperature (HT) form] and the Dy3Ni2-type [the low-temperature (LT) form].10 Since the existence of the ‘Gd3Ni2’ phase remains doubtful, yet such a material would be of potential interest as a magnetic refrigerant material, a thorough investigation of its formation and stoichiometry is warranted.13
In this work we report the crystal structure, thermal stability, magnetic behavior and magnetocaloric effect (MCE) of Gd3Ni2 and substituted Gd3CoxNi2−x phases for 0 < x ≤ 1.0. Electronic structure calculations have been performed to understand the preferential Co/Ni site occupations leading to the confirmation of the ternary Gd3CoNi ordered derivative and the magnetic behaviors of these compounds.
The X-ray powder patterns were indexed, with the help of Lazy PULVERIX,15 on the basis of the monoclinic Dy3Ni2 prototype [mS20, C2/m (No. 12), Z = 4].10 The lattice parameters (a, b, c, and β), unit cell volume (Vobs) and volume of formation {−ΔV %, where ΔV = [(Vcalc − Vobs)/Vcalc × 100]; Vcalc is the volume of the compound calculated from the atomic volumes of the individual atoms21} for Gd3Ni2 are reported in Table 1. The lattice parameters are larger than those of the other known Dy3Ni2-type R3Ni2 phases (R = Tb, Dy, hT-Ho),10 and are in agreement with the trend of the lanthanide contraction. The volume of formation observed for Gd3Ni2 (≈ −4.7%) is relatively small compared to the values obtained for other Gd–Ni compounds and several binary and ternary Gd phases,5,6 suggesting that a considerably low atomic space filling takes place in the formation of this compound. This result prompted us either to investigate pseudo-binary alloys by substituting either Gd by a larger R (e.g. Nd), or Ni by a larger transition element (e.g. Co, Pd), or by the addition of a small interstitial element (e.g. B, C), to check if the Dy3Ni2 structure type was preserved, and if the substitution could stabilize the formation of this phase. Co substitution was first attempted because of its similarity to Ni (the atomic volumes are 11.08 Å3 and 10.93 Å3 for Co and Ni, respectively21). Samples with nominal composition Gd3CoxNi2−x (for x = 0.25, 0.50, 0.75, 0.85, 0.95, 1.00) were prepared and studied. As a first result, we found that the Co substitution for Ni stabilizes the pseudo-binary Gd3CoxNi2−x phases down to room temperature; the alloy with the lowest Co content, i.e. Gd60Co5Ni35 ≡ Gd3CoxNi2−x with x = 0.25 was still a single phase with the Dy3Ni2-type structure after annealing at 673 K (well below the eutectoid decomposition temperature of pure Gd3Ni2) for 18 days. An X-ray powder diffraction pattern of Gd60Co15Ni25, along with its Rietveld profile, is shown as an example in Fig. 1. Moreover, the monoclinic prototype is preserved up to the composition Gd3CoNi (x = 1.0). When x exceeds 1, the crystal structure changes to the orthorhombic Y3Co2 prototype [oP20, Pnnm (No. 58), Z = 4]. The two prototypes – Dy3Ni2 and Y3Co2 – are closely related to one another via displacements of slabs common to both structures,22 which are similar to the relationships between CrB-, FeB-, and TbNi-type structures. All the substituted Gd3CoxNi2−x phases also form via peritectic reactions, at temperatures slightly, but progressively, decreasing with increasing Co content [from 988 K (715 °C) for Gd3Ni2 to 981 K (708 °C) for Gd3Co0.75Ni1.25 and 975 K (702 °C) for Gd3CoNi]. A DSC trace for Gd3CoNi alloy is shown in Fig. S1 in the ESI.†
Gd3CoxNi2−x | Co [at%] | Lattice parameters | V obs [Å3] | V at [Å3] | −ΔV [%] | |||
---|---|---|---|---|---|---|---|---|
a [Å] | b [Å] | c [Å] | β [°] | |||||
Lattice parameters for Gd3Ni2 are those from a sample annealed at 953 K for 6 days and quenched in water. | ||||||||
Gd3Ni2 | 0 | 13.419(3) | 3.720(1) | 9.640(2) | 106.250(3) | 461.97 | 23.10 | 4.68 |
Gd3Co0.25Ni1.75 | 5 | 13.420(2) | 3.7358(5) | 9.6000(9) | 106.738(11) | 460.90 | 23.04 | 4.93 |
Gd3Co0.50Ni1.50 | 10 | 13.4160(9) | 3.7529(3) | 9.5708(5) | 107.385(5) | 459.87 | 22.99 | 5.17 |
Gd3Co0.75Ni1.25 | 15 | 13.408(1) | 3.7796(5) | 9.5464(5) | 108.128(7) | 459.78 | 22.99 | 5.22 |
Gd3Co0.85Ni1.15 | 17 | 13.405(1) | 3.7895(6) | 9.537(1) | 108.481(8) | 459.50 | 22.97 | 5.29 |
Gd3Co0.95Ni1.05 | 19 | 13.402(2) | 3.803(1) | 9.534(1) | 108.828(2) | 459.89 | 22.99 | 5.22 |
Gd3CoNi | 20 | 13.400(2) | 3.810(1) | 9.537(2) | 109.028(2) | 460.33 | 23.02 | 5.13 |
In Gd3CoxNi2−x both a and c decrease, while b and β increase with x, and the unit cell volume slightly decreases (Fig. 2, Table 1). Since the atomic volume of elemental Co is slightly larger than that of Ni, one would have expected the opposite – an increase of the unit cell volume with increasing Co content. The observed decrease may be due to either the fact that Co assumes an anomalously large volume in its elemental form, and when alloyed it behaves as a normal 3d metal with a smaller atomic volume than Ni,23 or to the peculiar site preference of Co atoms (see next section). The absolute value of the volume of formation (|ΔV| %) in these compounds sensibly increases with the Co content (Fig. 2); since the volume of formation is proportional to the thermodynamic stability (heat of formation) of the compound,24,25 such an increase across the Gd3CoxNi2−x series supports the notion of a higher stability brought about as a result of Co substitutions. At the same time, the trends illustrated in Fig. 2 suggest that the unit cell will not sustain a higher Co substitution while preserving the same monoclinic Dy3Ni2-type structure. A structural change to the orthorhombic Y3Co2-type for x > 1.0 is in fact observed; this will be the subject of a future study.
Compound | Gd3Ni2 | Gd3CoNi |
---|---|---|
Structure prototype | Dy3Ni2 | Dy3Ni2 |
Pearson code | mS20 | mS20 |
Crystal system | Monoclinic | Monoclinic |
Space group | C2/m (No. 12) | C2/m (No. 12) |
Lattice parameters | a = 13.445(3) Å | a = 13.407(2) Å |
b = 3.7270(7) Å | b = 3.8118(7) Å | |
c = 9.646(2) Å | c = 9.5351(19) Å | |
β = 106.44(3)° | β = 109.079(10)° | |
Unit cell volume [Å3] | 463.6(2) | 460.51(14) |
Unit formula per cell, Z | 4 | 4 |
Absorption coefficient, μ (Mo Kα) [mm−1] | 50.078 | 49.927 |
Calculated density, ρ [g cm−3] | 8.441 | 8.501 |
F(000) | 992 | 988 |
Crystal size [mm] | 0.08 × 0.06 × 0.06 | 0.11 × 0.08 × 0.12 |
Theta range [°] | 3.16 ≤ θ ≤ 26.66 | 2.26 ≤ θ ≤ 27.50 |
Range in h, k, l | −15 ≤ h ≤ 15, −4 ≤ k ≤ 4, 0 ≤ l ≤ 12 | −17 ≤ h ≤ 17, −4 ≤ k ≤ 4, −11 ≤ l ≤ 12 |
Measured reflections | 900 | 1659 |
Independent reflections | 527 | 597 |
Absorption correction | Empirical | Empirical |
Refinement method | Full-matrix least-squares on F2 | Full-matrix least-squares on F2 |
Refined parameters | 32 | 32 |
Data/restraints/parameters | 527/0/32 | 597/0/32 |
R1 all data, wR2 (Fo2) all data | 0.0619, 0.0685 | 0.0389, 0.1096 |
R1, wR2 (Fo2) [I > 2 σ(I)] | 0.0379, 0.0633 | 0.0315, 0.0755 |
R int | 0.035 | 0.029 |
Goodness-of-fit | 1.037 | 1.234 |
Δρmax, Δρmin, e Å−3 | +1.925, −2.815 | +2.605, −2.196 |
Atom | Atomic coordinates | U eq [Å2] | ||
---|---|---|---|---|
x | y | z | ||
Gd3Ni2 | ||||
Gd1 | 0.36797(9) | 0 | 0.0018(1) | 0.0157(3) |
Gd2 | 0.0971(1) | 0 | 0.6728(1) | 0.0164(3) |
Gd3 | 0.35598(9) | 0 | 0.6295(1) | 0.0167(3) |
Ni1 | 0.03578(3) | 0 | 0.1432(3) | 0.0210(7) |
Ni2 | 0.24231(3) | 0 | 0.2268(3) | 0.0220(7) |
Gd3CoNi | ||||
Gd1 | 0.36691(8) | 0 | 0.0009(1) | 0.0106(4) |
Gd2 | 0.10373(9) | 0 | 0.6773(1) | 0.0118(4) |
Gd3 | 0.36179(8) | 0 | 0.6260(1) | 0.0115(4) |
Ni | 0.0354(3) | 0 | 0.1425(4) | 0.0173(7) |
Co | 0.2378(2) | 0 | 0.2371(4) | 0.0161(7) |
Because of their close electronegativities (1.88 for Co and 1.91 for Ni, Pauling scale) and atomic size, Co and Ni frequently occupy the same crystallographic sites forming solid solutions leading generally to fully or partially disordered structures. The high quality of the Gd3CoNi crystals allowed us to distinguish fully occupied Co and Ni positions. Slightly better R-values (statistically significant, according to the Hamilton test27) and, more importantly, uniform thermal displacement parameters were obtained by setting Ni and Co as listed in Table 3. The opposite distribution of Ni and Co (different coloring scheme) leads to Ueq = 0.0160(7) and 0.0207(6) for Co and Ni, respectively. In the intermediate Gd3CoxNi2−x phases, Co gradually replaces Ni at the Ni2 site of the parent compound, up to the full occupancy in Gd3CoNi; hence the 3:1:1 stoichiometric compound corresponds to the Co-rich limit of the series adopting the Dy3Ni2-type. Since the difference in atomic size and electronegativity between Ni and Co is nearly negligible, the crystallographic ordering of these atoms must be primarily controlled by the electronic factors.
A sketch of the crystal structure of both Gd3Ni2 and Gd3CoNi compounds is shown in Fig. 3a and b, respectively, where the ordered arrangement of the Co atoms is highlighted. The structure is represented by a trigonal-prismatic arrangement of the smaller atoms, forming columns of four face-sharing blocks along the shortest crystallographic axis, b. The trigonal prisms are centered by Ni atoms in Gd3Ni2, or by Co/Ni atoms in Gd3CoNi (Fig. 3c and d).
A comparison of the interatomic distances indicates that some values clearly decrease in Gd3CoNi when compared to Gd3Ni2 (Tables S2 and S3, ESI†). Since all these values are lower than the sum of their corresponding metallic radii, ∑rM, (where rM = 1.802 Å, 1.252 Å and 1.246 Å for Gd, Co and Ni, respectively),28 it is reasonable to consider them as bond distances. The shortest Gd2–Ni2 distance in the Gd3Ni2 structure δGd2–Ni2 = 2.809 Å (−7.8%) contracts to δGd2–Co = 2.771 Å (−9.3%) in Gd3CoNi. The shortest Gd–Gd interatomic distances, 3.548–3.727 Å for Gd3Ni2 (−1.6% to +3.4% with respect 2rGd = 3.604 Å) and 3.574–3.854 Å for Gd3CoNi (−2.8% to +5.8%, respectively), show relatively weak Gd–Gd interactions. Upon the transition from Gd3Ni2 to Gd3CoNi, the Gd1–Gd2 and Gd1–Gd3 distances decrease from 4.098 Å to 3.854 Å and from 4.353 Å to 4.175 Å, respectively, while the Gd1–Gd1, Gd2–Gd2, and Gd3–Gd3 increase from 3.727 Å to 3.812 Å; the other Gd–Gd distances remain practically constant (<1.2%). Weak Ni–Ni, or Ni–Co, chemical bonds are also formed in both compounds (Tables S2 and S3, ESI†).
To better understand the distribution of the neighboring atoms around Gd, Co and Ni in these two phases, we used criteria described by Bruzzone et al.29 In this approach, the atomic distribution around one given atom is described by plotting the number of its surrounding atoms, placed at a certain distance d, against the ratio dobs/∑rM (where dobs is the observed interatomic distance between two next-neighbor atoms, and ∑rM is the sum of the two metallic radii),29 where only neighboring atoms up to values dobs/∑rM ≤ 1.25 should be considered. The histograms for all atoms in both compounds are shown in Fig. S2 (ESI†). Since the distributions of the interatomic distances do not show clear gaps useful for the unambiguous separation of the bonding and non-bonding distances, the dobs/∑rM ≤ 1.25 criterion has been applied (we note that bonding/non-bonding distance differentiation is quite common in the chemistry of rare-earth compounds30,31). The determined coordination polyhedra around all atoms are shown in Fig. 4. In both Gd3Ni2 and Gd3CoNi compounds the atomic distribution around Gd atoms indicates large and distorted polyhedra with relatively high coordination numbers, CN, of 14, 16, and 17. The coordination polyhedra for Ni1 and Ni2/Co2 are distorted tricapped trigonal prisms (CN = 9, Fig. 4). The distortion decreases with increasing Co content due to the shortening of the Gd3–Co distance.
Fig. 4 Coordination polyhedra of the Gd, Co and Ni atoms in the Gd3CoNi compound (for interatomic distances dobs/∑rM ≤ 1.25). |
Fig. 6 Magnetization and inverse magnetic susceptibility measured in the range of 2–300 K and at 200 and 2000 Oe of Gd3Ni2 (a) and Gd3CoNi (b). |
Compound | Co | T C | θ P | μ eff | M sat | M sat (H → ∞)b |
---|---|---|---|---|---|---|
[at%] | [K] | [K] | [μB] | [μB per Gd] | [μB per Gd] | |
a Values for a field H = 70 kOe. b Extrapolated values. | ||||||
Gd3Ni2 | 0 | 147 | 166 | 8.35 | 7.00 | 7.0 |
Gd3Co0.25Ni1.75 | 5 | 150 | 169 | 8.37 | 7.00 | 7.0 |
Gd3Co0.5Ni1.5 | 10 | 154 | 175 | 8.30 | 7.18 | 7.2 |
Gd3Co0.75Ni1.25 | 15 | 163 | 183 | 8.39 | 7.47 | 7.5 |
Gd3Co0.85Ni1.15 | 17 | 168 | 186 | 8.44 | 7.44 | 7.5 |
Gd3Co0.95Ni1.05 | 19 | 172 | 190 | 8.44 | 7.43 | 7.5 |
Gd3CoNi | 20 | 176 | 194 | 8.32 | 7.37 | 7.5 |
The isothermal magnetization, M(H), was measured at 2, 5, 10 and 120 K for Gd3Ni2 (Fig. 8a shows the data at 5 and 120 K) and at 5 K for Gd3CoNi (Fig. 8b) and the Gd3CoxNi2−x phases for x = 0.50, 0.75, 0.85, 0.95 (Fig. S4, ESI†), in fields up to 70 kOe. At 5 K, well below the TC, the hysteresis loops for all these phases are characteristic of soft ferromagnets, with negligible a remanence and a coercive field (HC of 5–10 Oe). For Gd3Ni2 the magnetization saturates at 8 kOe, with a saturation moment of 7.0 μB per Gd; for the substituted Gd3CoxNi2−x the magnetization is already almost saturated at a field of 5–6 kOe. The saturation moments in the Co containing phases sensibly, and progressively, increase from 7.0 to about 7.4 μB per Gd (Table 4). While the saturation moment found for Gd3Ni2 corresponds to the theoretical value of the free Gd3+ ion, the values for the substituted Gd3CoxNi2−x compounds are slightly higher resulting from 3d–5d hybridization.
The temperature dependence of the magnetic entropy change for magnetic field changes (ΔH) of 10, 20, 30, 40 and 50 kOe in Gd3Ni2 and Gd3CoNi is shown in Fig. 10a and b, respectively (Fig. S5e and f for Gd3Co0.75Ni1.25 and Gd3Co0.85Ni1.15, respectively, ESI†). In all compounds, the maximum value of −ΔSM is observed around the TC. The magnetocaloric effect increases slightly with increasing Co content: from 2.1 J kg−1 K−1 in Gd3Ni2 to 2.3 J kg−1 K−1 in Gd3CoNi for ΔH = 10 kOe, or from 8.0 J kg−1 K−1 in Gd3Ni2 to 8.3 J kg−1 K−1 in Gd3CoNi for ΔH = 50 kOe (Table S4, ESI†). These compounds exhibit relatively large magnetic entropy changes at intermediate temperatures compared with values generally found for a second order transition. The Arrott plots of these compounds (corresponding to the isothermal magnetization measurements plotted as M2vs. the ratio H/M)39 show a positive slope around the TC (Fig. 9c, d and Fig. S5c, d, ESI†), thereby confirming a second order transition in these phases. The magnetic entropy change as a function of the applied magnetic field increases nearly proportionally to H2/3, as expected from the mean field theory (Fig. 11).
Fig. 10 Temperature dependence of the magnetic entropy change (−ΔSM) in Gd3Ni2 (a) and Gd3CoNi (b) for ΔH = 10, 20, 30, 40, 50 kOe. |
Fig. 11 Maximum isothermal magnetic entropy change (−ΔSM at TC) vs. the applied magnetic field for Gd3Ni2 and Gd3CoNi. |
The magnetic entropy change is not the only parameter to characterize the potential of a magnetic refrigerant: the refrigerant capacity (RC), or cooling power,40 is another often employed important variable. The refrigerant capacity quantifies the efficiency of a magnetic material in terms of the energy transfer between the cold and the hot reservoir in an ideal thermodynamic refrigeration cycle. It measures how much heat can be transferred between the hot and the cold ends; so, for practical applications, a large RC over a wide temperature range coupled with a substantial magnetocaloric effect is desirable. For the Gd3Ni2, Gd3Co0.75Ni1.25, Gd3Co0.85Ni1.15 and Gd3CoNi compounds, the RC values have been calculated by integrating the area of the −ΔSMvs. T curves (between T1 and T2) by using the following equation:40
It may also be interesting to compare the magnetocaloric properties of Gd3Ni2 and Gd3CoxNi2−x compounds with those of other potential magnetic refrigerants. The magnetic entropy change, −ΔSM, of these materials of ≈ 4.0 J kg−1 K−1 for ΔH = 20 kOe is slightly smaller than that reported for Gd metal (5.1 J kg−1 K−1; TC = 298 K), or the dialumide GdAl2 (4.2 J kg−1 K−1, TC = 167 K)41 and much smaller than that of Gd5Si2Ge2 (14.1 J kg−1 K−1, TC = 299 K)42 for the same field change of 20 kOe. At the same time, this value is higher than that observed in other Gd-based intermetallics, such as Gd3Al2 (3.6 J kg−1 K−1 for ΔH = 11 kOe; TC = 281),43 Gd7Pd3 (2.5 J kg−1 K−1 for ΔH = 20 kOe; TC = 323 K)44 and GdScGe (1.45 J kg−1 K−1 for ΔH = 15 kOe; TC = 350 K)45. On the other hand, the values of refrigerant capacity observed for Gd3Ni2 and Gd3CoNi are 153 and 180 J kg−1, respectively, for a ΔH = 20 kOe (540 and 545 J kg−1, respectively, for a ΔH = 50 kOe). These values compare favorably with other RCFWHM data reported for most Gd intermetallics with a TC around room temperature, but are even higher than for compounds with a lower TC, thus making them potential candidates for intermediate-temperature magnetic refrigerant materials.
Fig. 12 shows atom projected 4f, 5d and 3d density of states of Gd3Ni2 and Gd3CoNi. The energy-band centers of occupied 4f density of states (DOS) of the three non-equivalent Gd atoms (Fig. 12a and d) slightly change when Ni at the Ni2 site of Gd3Ni2 is replaced by Co. This is likely due to the slight change in the Gd positions and, consequently, in the Gd–Gd distances while substituting Ni2 by Co. The unoccupied 4f DOS in both compounds is ≈4 eV above the Fermi level (not shown). The 5d DOS of non-equivalent Gd atoms in Gd3Ni2 is exchange-split by ≈ 0.2 eV between spin-up and spin-down 5d states across the Fermi level (Fig. 12b). Identical exchange splitting across the Fermi level is also observed in the 3d density of states of Ni atoms in Gd3Ni2 (Fig. 12c). This indicates that the Gd 5d and Ni 3d bands are hybridized in this compound. The Ni 3d magnetic moments are less than 0.03 μB, i.e. they are negligible compared to the Gd 5d moments. The magnetic moments of the three non-equivalent Gd1, Gd2, and Gd3 in Gd3Ni2 are 7.36 μB, 7.45 μB, and 7.47 μB, respectively. The ≈ 7 μB are from 4f moments and the remaining are from spin polarized 5d electrons due to the indirect 4f–4f exchange interactions. On the other hand, in Gd3CoNi the calculations show an exchange splitting of ≈ 0.5 eV between spin-up and spin-down Gd 5d and Ni/Co 3d states across the Fermi level (Fig. 12e and f). The Gd1, Gd2, Gd3 and Ni1 magnetic moments essentially remain identical to those of Gd3Ni2. Although Co moments (−0.34 μB) align antiparallel to Gd moments as expected, the enhanced Gd 5d and Ni/Co 3d exchange splitting at the Fermi level supports the experimentally observed enhancement of the Curie temperature in Gd3CoNi compared to Gd3Ni2 and may account for a larger than expected moment.
Fig. 12 (a) and (d) Gd 4f, (b) and (e) Gd 5d, and (c) and (f) Ni/Co 3d density of states (DOS) of Gd3Ni2 and Gd3CoNi compounds, respectively. |
Both Gd3Ni2 and Co-substituted phases exhibit similar magnetic behaviors: a long range ferromagnetic order sets in at TC values progressively increasing from 147 K (for Gd3Ni2) to 176 K (for Gd3CoNi). Saturation moments of 7.0 μB per Gd for Gd3Ni2 and 7.0–7.4 μB per Gd for the Gd3CoxNi1−x phases have been found. The increase in the saturation magnetic moment from Gd3Ni2 to Gd3CoNi reflects the enhanced contribution from 5d electrons of Gd. Reversible and soft ferromagnetism of these compounds, with negligible hysteresis, makes these new Gd-based intermetallics potentially useful magnetic refrigerant materials at intermediate temperatures.
Total energy calculations confirm the observed crystallographic site preference of Co and Ni atoms in Gd3CoNi. The enhanced Gd 5d and Ni/Co 3d exchange splitting at the Fermi level supports the experimentally observed enhanced Curie temperature in Gd3CoNi compared to that of Gd3Ni2. These new compounds constitute a potentially interesting source for investigation in both theoretical and experimental research. These new phases deserve further investigation to probe the effect of Gd substitution by another R (e.g. Nd) and/or Ni by a different transition metal (or a p-block element), with the aim of either tuning the TC or enhancing the MCE.
Footnote |
† Electronic supplementary information (ESI) available. CCDC 1458711 and 1458712. For ESI and crystallographic data in CIF or other electronic format see DOI: 10.1039/c6tc01035k |
This journal is © The Royal Society of Chemistry 2016 |