Open Access Article
This Open Access Article is licensed under a
Creative Commons Attribution 3.0 Unported Licence

Single ion magnets based on lanthanoid polyoxomolybdate complexes

José J. Baldoví a, Yan Duan a, Carlos Bustos bc, Salvador Cardona-Serra d, Pierre Gouzerh c, Richard Villanneau c, Geoffrey Gontard c, Juan M. Clemente-Juan a, Alejandro Gaita-Ariño *a, Carlos Giménez-Saiz *a, Anna Proust *c and Eugenio Coronado *a
aInstituto de Ciencia Molecular (ICMol), Universidad de Valencia, C/Catedrático José Beltran, 2, E-46980 Paterna, Spain. E-mail: alejandro.gaita@uv.es; carlos.giménez@uv.es; eugenio.coronado@uv.es
bFacultad de Ciencia, Instituto de Química, Campus Isla Teja, Universidad Austral de Chile, Valdivia, Chile
cSorbonne Universites, UPMC-Paris 06, UMR 8232, Institut Parisien de Chimie Moléculaire, 4 Place Jussieu, F-75005 Paris, France. E-mail: anna.proust@upmc.fr
dTrinity College Dublin, College Green, Dublin 2, Ireland

Received 6th June 2016 , Accepted 24th August 2016

First published on 25th August 2016


Abstract

Polyoxometalate (POM) chemistry has recently offered excellent examples of single ion magnets (SIMs) and molecular spin qubits. Compared with conventional coordination compounds, POMs provide rigid and highly symmetric coordination sites. However, all POM-based SIMs reported to date exhibit a very limited range of possibilities for chemical processability. We present herein two new families of POM-based SIMs which are soluble in organic solvents: [Ln(β-Mo8O26)2]5− {LnIII = Tb, Dy, Ho, Er, Tm and Yb} and the functionalised POMs [Ln{Mo5O13(OMe)4NNC6H4-p-NO2}2]3− {LnIII = Tb, Dy, Ho, Er, Yb and Nd}. In addition, these two families represent the first SIMs based on polyoxomolybdates. A magneto-structural analysis of these families is presented, which is based on an effective crystal field model, and compared with the results reported in analogous lanthanoid SIMs based on polyoxotungstates.


Introduction

The main goal of spintronics is the active manipulation of the electron spin degrees of freedom in solid-state systems for carrying information.1,2 Spintronic systems have experienced a rapid development and currently are used in a range of applications, including read-heads devices and non-volatile magnetic memories (MRAM).3,4 Extraordinary potential for these systems is expected for the fabrication of spin-transfer nano-oscillators (STNOs)5 and quantum computers.6–8 The progress of molecular electronics and molecular magnetism has led to the emergence of a new field known as molecular spintronics,9,10 which combines the ideas and concepts of spintronics with the singular possibilities offered by molecular electronics and molecular magnetism to develop a second generation of spintronic devices.11–14

A particularly challenging area within this field is that of single-molecule spintronics, which intends to use individual molecules as main components of spintronic devices. In this context, single-molecule magnets (SMMs)15 have been proposed as promising candidates.16–18 These systems, which represent the limit of miniaturization of nanomagnets, are between the most complex magnetic entities, exhibiting slow relaxation of the magnetization19 and magnetic hysteresis20 at liquid-helium temperatures. Moreover, they may also present quantum phenomena from purely molecular origin.21–24 In this context, SMMs based on mononuclear lanthanide complexes deserve a special attention.25,26 The first example of this class of molecular nanomagnets, also known as single-ion magnets (SIMs), was reported by Ishikawa and co-workers in the series with general formula [LnPc2], where lanthanoid ions are sandwiched between two phthalocyaninato moieties displaying a square-antiprismatic D4d symmetry.27 Derivatives closely related to this family include the oxidised terbium phthalocyaninato complex [TbPc2]0. This system, besides its “double-decker” structure which favours adsorption on surfaces, is electrically neutral. This feature facilitates its sublimation under UHV conditions. The processability of lanthanoid phthalocyaninato complexes has allowed a series of breakthroughs including the realization of molecular/supramolecular spin valves28,29 and the electrical control of nuclear spin qubits.30,31 Indeed, sublimable lanthanoid complexes have demonstrated a great potential in molecular spintronics. Among the few sublimable lanthanoid-based systems reported so far, we can highlight the trinuclear Tb3+ complex Tb3(OQ)9 (OQ = quinolinato), where spin-polarised hopping transport has been realised.32 It has also been proposed as a model system for quantum error correction in quantum computing.33

A second series of SIMs is that provided by polyoxometalate (POM) chemistry,34 a class of systems that has produced a number of conventional SMMs.35,36 In this case, mononuclear lanthanoid complexes encapsulated by POMs have produced key examples of spin qubits for quantum computing. Indeed, extended quantum coherence was recently achieved on concentrated samples of the holmium derivative of the series [Ln(W5O18)2]9− (in short LnW10) through the use of atomic clock transitions.37 Employing a different strategy, a large number of coherent manipulations was realised in the Gd3+ derivative38 of the [LnP5W30O110]12− series (in short LnW30).39 Within the same POM family, current rectification was achieved in a single molecule diode of DyW30.40 Still, the incorporation of these molecular inorganic polyanions onto surfaces or its anchoring to electrodes have been limited by their poor solubility in organic solvents and by their difficult functionalization with organic ligands.

Here, we have prepared two families of POM-based mononuclear lanthanide complexes with a rigid square antiprism structure, analogous to that of LnW10, which overcome these processing limitations. The first family is formulated as [Ln(β-Mo8O26)2]5− (in short, LnMo16), {LnIII = Tb, Dy, Ho, Er, Tm and Yb} and consists of a lanthanide ion trapped by two [β-Mo8O26]4− moieties.41 The second family is formulated as [Ln{Mo5O13(OMe)4NNC6H4-p-NO2}2]3− (in short, LnMo10), {LnIII = Tb, Dy, Ho, Er, Yb and Nd}. In this cases the lanthanide ion is trapped by a functionalised POM based on a lacunary Lindqvist-type pentamolybdate.42

Results and discussion

Solubility and stability

LnMo16 series. The LnMo16 series are very soluble in acetone, acetonitrile and benzonitrile. Their derivatives are insoluble in methanol, ethanol, dichloromethane or chloroform, giving rise to colorless solutions. The structural integrity of the POMs in solution is kept as long as the solvents are dried, as shown by electrospray ionization for acetonitrile solutions (see Fig. S6). Wet solvents, however, give rise to yellow solutions, evidencing decomposition.
LnMo10 series. Owing to the structural analogy between the [Mo5O13(OCH3)4NNC6H4-p-NO2]3− units with their nitrosyl [Mo5O13(OCH3)4(NO)]3− analogues, one could a priori expect the transformation of the LnMo10 family of compounds in other solvents than methanol, in which they are synthesised. However they proved to be unexpectedly stable in several organic solvents at least at room temperature. Indeed, they are soluble and can be recrystallised in acetonitrile and chlorinated solvents (chloroform or dichloromethane) without noticeable decomposition, at the difference of their nitrosyl analogues.43 The combination of the stability and solubility properties of these compounds (the solution we used for their recrystallization are about 10−2 mol L−1) make them particularly interesting in the frame of their processing and utilization in nanodevices.

Crystal structures

LnMo16 series. This family of compounds crystallise in two different space groups: monoclinic (P21/c) for Tb3+ and orthorhombic (Pbca) for the rest of the series. Because of the rigidity of the POM, this difference in the crystallographic space group is in practice not noticeable in the vicinity of lanthanide ion. Thus, in all cases the structure exhibits the presence of a lanthanide ion sandwiched between two [β-Mo8O26]4− units. The lanthanide ions are coordinated by the eight terminal oxygen atoms coming from the two octamolybdate units giving rise to an eight-fold square antiprismatic coordination (Fig. 1). The structural parameters concerning the lanthanide coordination sphere are listed in Table 1. Details of the crystal structure determination and crystallographic parameters (Table S1) are given in the ESI.
image file: c6dt02258h-f1.tif
Fig. 1 (Left) Polyhedral and ball-and-stick representation of LnMo16 series and (right) projection of the coordination sphere showing the square-antiprismatic coordination site.
Table 1 Structural parameters concerning the lanthanide coordination sphere
  LnMo16 LnMo10
d pp[thin space (1/6-em)]a (Å) d in[thin space (1/6-em)]b (Å) φ (°) d pp[thin space (1/6-em)]a (Å) d in[thin space (1/6-em)]b (Å) φ (°)
a d pp defines the average distance between two oxygen based square planes. b d in is the average O–O distance within the oxygen-based square planes. c φ is defined as the relative orientation between the two squares defined by the coordinating oxygen atoms.
Tb 2.604(13) 2.853(15) 40.2(5) 2.661(8) 2.816(8) 44.1(2)
Dy 2.552(18) 2.844(18) 44.1(5) 2.640(6) 2.797(6) 44.2(2)
Ho 2.553(10) 2.825(10) 44.3(3) 2.638(5) 2.786(5) 39.2(7)
Er 2.551(11) 2.819(11) 44.2(3) 2.614(6) 2.783(6) 40.0(6)
Tm 2.506(14) 2.818(14) 44.1(4)
Yb 2.506(14) 2.796(14) 44.3(4) 2.585(6) 2.759(6) 39.3(7)


LnMo10 series. As in the case of the LnMo16 series, these complexes display a weakly distorted square antiprism geometry, in which the central Ln3+ cation interacts with two [Mo5O13(OMe)4(NNC6H4-p-NO2)]3− units playing the role of planar tetradentate ligands, and providing an eight-coordination environment. The structural parameters concerning the lanthanide coordination sphere are listed in Table 1. The geometrical parameters of this series are comparable to those observed for the nitrosyl derivatives [X{Mo5O13(OMe)4(NO)}2]n {X = Ca2+, Sr2+, Ba2+, Ce3+, Eu3+ and Bi3+},44 thus indicating a slightly distorted D4d geometry. The TbMo10 crystal structure is shown in Fig. 2. Details of the crystal structure determination and crystallographic parameters (Table S2) are provided in the ESI.
image file: c6dt02258h-f2.tif
Fig. 2 Polyhedral and ball-and-stick representation of the LnMo10 series.

Magnetic properties

LnMo16 series. A simultaneous fit was performed on the four magnetic susceptibility curves of the Tb3+, Dy3+, Ho3+ and Er3+ derivatives of this series using an effective crystal field approach (REC model; see section on experimental methods for details). The determined two parameters were tested by applying them to the real coordinates of the Tm3+ and Yb3+ derivatives. The predicted magnetic behaviour shows a very good agreement with the experimental data (Fig. 3).
image file: c6dt02258h-f3.tif
Fig. 3 Temperature-dependent magnetic susceptibility of the series LnMo16 and theoretical calculations using the REC model: Dy3+ (red), Ho3+ (blue), Tb3+ (pink), Er3+ (green), Tm3+ (black), Yb3+ (orange). Markers give experimental data under a magnetic field of 1000 Oe, and solid lines theoretical results: fits for Tb3+–Er3+ and predictions for Tm3+ and Yb3+.

The most satisfactory agreement was obtained when the radial displacement (Dr) equals 0.72 Å and the effective charge (Zi) is 0.253. If we compare the obtained parameters with the ones extracted in the families LnW10 and [Ln(β2-SiW11O39)2]13− (in short: LnW22),45 the radial displacement is smaller in this case. This means that the effective point charge needs a smaller covalent correction to produce an adequate relation between the crystal-field parameters that describe the experimental data. This difference can be related to the different Pauling electronegativity of the Mo and W atoms (2.16 and 2.36 respectively).46 The larger difference in electronegativity between Mo (2.16) and O (3.44) enhances the ionic character of the Mo–O bonding and also the coordination bond Ln–O.

The resulting energy levels for all the series are reported in the ESI (Fig. S10). A general trend for LnMo16 compared with LnW10 and LnW22 is a slightly larger crystal field splitting. In average, the Ln–O distance is practically identical in both series, e.g. in ErW10 and ErMo16 (2.367(7) Å and 2.367(3) Å). This would mean that polyoxomolybdates tend to produce a slightly stronger ligand field splitting compared with polyoxotungstates at a given metal–ligand distance. For a deeper analysis of the compounds that exhibit SMM properties in both families, the Stark sublevels of the HoMo16 and ErMo16 derivatives are plotted in Fig. 4. Regarding the lower states wave functions, one can observe that in the case of the HoMo16 the ground state is defined by a mixture of 47% of |+4> and 47% of |−4>. In this case, the crystal field operators enable a quantum tunnelling splitting between wave functions with a strong mixture of MJ components, and thus in absence of an external magnetic field no blocking of the magnetic moment is to be expected. Nevertheless when a longitudinal external field is applied, the purity of the MJ = +4 and MJ = −4 is recovered and thus, relaxation via tunnelling is cancelled and a blocking of the magnetization is possible. For ErMo16 the wave function for the ground state appears to be MJ = 0.78|±1/2> + 0.12|±13/2> with two states lying closely above it (at about 1.6 and 3.7 cm−1). Those are described by MJ = 0.78|±15/2> –marked in red in Fig. 4– and MJ = 0.74|±13/2> + 0.15|±15/2> respectively. The low energy difference between the ground and the first excited state (and even the second) is definitively below the precision of the method. Also, thermal effects over the chemical structure, while only slightly affecting the energy level description,47 are expected to become significant. This is expected to affect our modelling of the magnetization. As seen below, it is likely from the dynamic susceptibility behaviour that the Kramers doublet described by 78% of ±15/2 is the actual ground doublet. Within this assumption, the ground wave function would show a high MJ projection compatible with SMM behaviour.


image file: c6dt02258h-f4.tif
Fig. 4 Energy level scheme and main contributions to the ground state wave function for HoMo16 and ErMo16.

The ac magnetic susceptibilities were collected in the range 2–12 K with an applied alternating field of 3.95 Oe at different frequencies in the range 1–10[thin space (1/6-em)]000 Hz. ErMo16 and HoMo16 show frequency dependent out-of-phase signals at very low temperatures. In neither complex a clear peak is observed (Fig. S2 and S3) even under an external applied field of 1000 Oe. (Fig. 5 and 6) This feature is a characteristic of the fast relaxation process that takes place at low temperatures. In none of the other derivatives an increase in the out-of-phase signal down to 2 K was observed.


image file: c6dt02258h-f5.tif
Fig. 5 In-phase (up) and out-of-phase (down) dynamic susceptibility of HoMo16 (left) and ErMo16 (right) with an applied field of 1000 Oe. The frequencies are shown in the legend. Solid lines are eye-guides.

image file: c6dt02258h-f6.tif
Fig. 6 Experimental (circles) and predicted (solid lines) χT product of the series LnMo10 under a magnetic field of 1000 Oe: Dy3+ (red), Ho3+ (blue), Tb3+ (pink), Er3+ (green), Yb3+ (orange), Nd3+ (clear blue) from 2 to 300 K.
LnMo10 series. For this series our initial prediction, based on the coordination geometry around the lanthanoid, pointed towards the possibility of obtaining SMM behaviour in the Dy derivative (97% of MJ = ±11/2), in Yb (97% of MJ = ±5/2) and in Er (99% of MJ = ±15/2) (see Experimental methods section). This was confirmed by the ac susceptibility data that showed slow relaxation of the magnetization in all three derivatives (Fig. 7, S4 and S5).
image file: c6dt02258h-f7.tif
Fig. 7 In-phase (up) and out-of-phase (down) dynamic susceptibility of DyMo10 (left) and YbMo10 (right) under an applied field of 1000 Oe. The frequencies are shown in the legend. Solid lines are eye-guides.

The REC model permits to characterize the magnetic and spectroscopic properties of a family of complexes using a range of approaches. An extreme limit is the rough prediction with no free parameters,48 which allows the discovery of new SIMs. On the opposite extreme, one can perform an individual fit for each metal, which describes the observables more accurately but has a more reduced ability to extrapolate the results to related derivatives. In this case, we have decided to employ an intermediate path. Owing to the chemical similarity of the two families of polyoxomolybdates presented in this work, especially in the coordination environment, the product of the parameters Dr = 0.72 Å and Zi = 0.253 obtained in the study of LnMo16 was used to reduce the number of independent REC parameters for each metal when modelling the magnetic properties of LnMo10. The magnetic susceptibility curves of this series were fitted individually keeping the relation f = Dr·Zr constant, allowing just one free parameter per compound. The results are plotted in Fig. 6, where we can observe the excellent agreement between the model and the experiment. The sharp decrease that appears in ErMo10 below 10 K is reminiscent of the behavior previously observed at the same temperature range in other complexes,49,50 such as [Er(COT)2], [Er(COT′′)2] and Er(Cp*COT), where COT = cyclooctatetraenyl dianion, COT′′ = 1,4-bis-(trimethylsilyl) cyclooctatetraenyl dianion and Cp* = pentamethylcyclopentadienide. As in the present case, in those examples the ground doublet can be characterized as an Ising state (MJ = ±15/2), and this may favour a stronger dipolar interaction at low temperature. The estimation of the energy levels (Fig. S8) and wave functions of this new family of polyoxomolybdates are reported in the ESI.

An analysis of the frequency dependence of the χ′′ peaks through Arrhenius plots (Fig. S6) has permitted to estimate the magnetization-relaxation parameters. Compared with analogous polyoxotungstates, polyoxomolybdates display poorer behaviour as SIMs. Out of the whole series, Dy3+, Er3+ and Yb3+ complexes can be characterised as SIMs (displaying clear peaks above 2 K) and only under an external dc field H = 1000 G. Under these conditions, a naïve fitting of the ac data of the Dy3+, Yb3+ derivatives assuming an Orbach process would result in a barrier height (Ueff/kB) of 38.5 K with a preexponential factor (τ0) of 6.6 × 10−8 s for the Dy3+ case and 23.3 K with τ0 = 6.7 × 10−6 s for the Yb3+ case, compared with the archetypical ErW10 (Ueff/kB) = 55.2 K and τ0 = 1.6 × 10−8 s. These plots do not contain enough information to independently fit a Raman process, but this should not be taken as a proof of an Orbach mechanism, especially lacking spectroscopic indication of levels at these energies. This is even more marked for the Er3+ derivative, which displays only two clear χ′′ peaks, precluding an Arrhenius fit.

The calculated energy level schemes for DyMo10, ErMo10 and YbMo10 are represented in Fig. 8. According to the individual magnetic susceptibility data fits based on the predictions of the REC model, DyMo10 possesses a ground state dominated by MJ = ±11/2 (86%) with an excited state of MJ = 0.92|±9/2>, which is placed at about 11 cm−1 above it. Such scheme is compatible with the observed SMM behaviour. One can notice that in this example all the MJ states are bunched below 100 cm−1 with the exception of the highest MJ = 15/2 which is located at 260 cm−1. In ErMo10, the ground state is characterised by 99% of MJ = 15/2 and the first excited Kramers doublet is placed at about 19 cm−1. In the case of YbMo10, the level scheme also supports the relationship between the ground-state wave function (described by MJ = 97% of |±5/2>) and the SMM behaviour. The rest of the energy levels appear at about 167 cm−1 above it, starting with the MJ = 0.69|±3/2>. The absence of mixing provides a quasi-pure MJ function in the ground state without a clear path to invert its moment, thus the magnetic moment may be blocked at low temperatures. Here one again needs to highlight the risk of an Orbach-only interpretation in absence of richer experimental information.


image file: c6dt02258h-f8.tif
Fig. 8 Energy level scheme and main contributions to the ground state wave function for DyMo10, ErMo10 and YbMo10.

Magneto-structural correlations

The optimization of f-element single-molecule magnets is still an open problem.26 Thus, at this point, it is worth to briefly compare the results of a given lanthanide ion as a function of the different ligand fields created in the different families of POMs showing an approximate D4d symmetry. For that, we will focus in the erbium analogue because its crystal structure has been determined for ErW10, ErW22, ErMo16 and ErMo10. Regarding the lowest energy levels, we found a ground state characterised by ±13/2 in both polyoxotungstates, and a first excited state dominated by ±1/2 (placed at about 16 cm−1 in ErW10 and 11 cm−1 in ErW22). In the case of ErMo10, the ground doublet is apparently dominated by ±15/2 (99%) and the first excited state (located at about 19 cm−1) presents 85% of ±1/2, according to our theoretical calculations based on available susceptibility data. The explanation of such a different energy scheme can be attributed to differences in the first coordination sphere, as well as differences in the effective charges and distances of the oxygen donor atoms. Thus, while in the two polyoxotungstate series the interplanar distances, dpp, are equal to 2.46 Å in ErW10 and 2.48 Å in ErW22, in the ErMo10 this distance increases to a value of 2.61 Å. ErMo16 represents an intermediate situation, having dpp = 2.55 Å and a skew angle comparable to that of ErW10 (44.2°). In this case, these inexpensive calculations indicate that there are three Kramers doublets very close in energy, two of them dominated by high MJ values and one dominated by ±1/2, being difficult to determine the true nature of the ground Kramers doublet.

Conclusions

In the last years, a sufficiently large set of lanthanoid-based SIMs has already been obtained. This has provided a good basis for relating their magnetic properties with the nature and structure of the coordination site around the lanthanide ion. A subsequent development that has been recently initiated is that related with the improvement in the chemical processability of these magnetic molecules in order to incorporate them into functional devices.

The present work contributes towards these two goals. Thus, we have used a robust family of ligands based on POMs to prepare new SIMs exhibiting SMM properties, which can be modelled using an effective crystal field approach previously developed for this kind of ligands. The key novelty has been the unprecedented use of polyoxomolybdates instead of polyoxotungstates for obtaining SIMs. While the chemistry of polyoxomolybdates is more challenging, this result has opened the possibility of making these magnetic molecules soluble in organic solvents, thus facilitating their processing and incorporation into devices. This contrasts with the SIMs based on polyoxotungstate ligands, which are commonly only soluble in water. Furthermore, we have also shown that polyoxomolybdate-based SIMs can be functionalised with organic groups, facilitating their processability -e.g. grafting onto surfaces/electrodes – and the incorporation of a second property coming from the organic ligand. Last but not least, the enhanced reduction potential of polyoxomolybdates may also be of interest to incorporate delocalised electrons into the mixed-valence POM framework, thus increasing the interest of these magnetic molecules in spintronics.51–54

Experimental methods

All reagents and solvents used were commercially available. Acetonitrile was distilled under argon before use. The precursor for the LnMo16 series: [TBA]4[β-Mo8O26], where TBA = (n-C4H9)4N was prepared according to a previously described literature procedure.55

The precursor [TBA]3[Mo6O18NN-C6H4-p-NO2] of the LnMo10 series was prepared as described elsewhere.56 The subsequent synthesis of the ligand [TBA]2[Mo5O13(MeO)4(NNC6H4-p-NO2){Na(MeOH)}] was slightly modified from the initial report (see below).42

Synthesis of LnMo16 series

The salts [TBA]5[Ln(β-Mo8O26)2] (LnIII = Tb, Dy, Ho, Er, Tm, and Yb) were prepared following a slight modification of a previously described procedure.43 A solution of lanthanide salt Ln(NO3)3 (0.200 mmol) in 5 mL of acetonitrile was added drop-wise to a solution of [TBA]4[β-Mo8O26] (0.376 mmol) in 25 mL of acetonitrile under stirring. Then, 50 mL of diethyl ether were added carefully, in such a way that two layers were formed. After three days of slow diffusion, block-shaped crystals formed and were collected by filtration, washed with a small amount of acetonitrile, and dried under vacuum overnight (see ESI for details of the elemental analysis and yield IR spectra).

Synthesis of LnMo10 series

Synthesis of the ligand [TBA]2[Mo5O13(MeO)4(NNC6H4-p-NO2){Na(MeOH)}]. [TBA]3[Mo6O18NN-C6H4-p-NO2] (1.740 g, 1.000 mmol) was introduced in 15 mL of methanol and 5 mL of 0.2 mol L−1 solution of NaOH in methanol (1 mmol) was then added. The mixture was heated in refluxing methanol (65 °C) for 1 hour, leading to a red limpid solution. This solution was then allowed to cool to room temperature and filtered on a glass frit (por. 4). Diethyl-ether (20 mL) was added to the resulting filtrate, which was then placed at −18 °C for one day. The red crystals thus obtained were filtered, rinsed with 3 portions of 5 mL of diethyl-ether and dried in air, yielding 1.200 g of [TBA]2[Mo5O13(MeO)4(NNC6H4-p-NO2){Na(MeOH)}].
Synthesis and crystallization of LnMo10 series. [TBA]2[Mo5O13(MeO)4(NNC6H4-p-NO2){Na(MeOH)}] (0.376 g, 0.250 mmol) was dissolved in 15 mL of methanol. 0.125 mmol of the lanthanide salt {TbCl3·6H2O: 0.048 g; ErCl3·6H2O: 0.0342 g; YbCl3·6H2O: 0.048 g; Dy(NO3)3·5H2O: 0.048 g; Nd(NO3)3·6H2O: 0.055 g; Ho(NO3)3·5H2O: 0.055 g} was then added. The resulting mixture was refluxed in methanol for 30 min. The red/orange precipitate formed after cooling the solution to room temperature was filtered on a glass frit (por. 4) and washed twice with diethyl-ether. All compounds were recrystallised by slow diffusion of diethyl-ether in a solution in chloroform (ca. 0.300 g in 15 mL of CHCl3), leading to the formation of dark red crystalline materials with general formula [TBA]3[Ln{Mo5O13(MeO)4NNC6H4-p-NO2}2]·1.5CHCl3.

Magnetic measurements

Magnetic static and dynamic measurements of samples of LnMo16 and LnMo10 were performed by compacted powder molded from ground crystalline samples. Variable-temperature susceptibility measurements were carried out under a magnetic field of 1000 Oe in the temperature range 2–300 K on a magnetometer equipped with a SQUID sensor (Quantum Design MPMS-XL-5). The data were corrected for diamagnetic contribution from eicosane and for the diamagnetic contributions of the polyanions as deduced by using the Pascal's constant tables. Isothermal magnetization measurements at low temperature (2 K) were performed up to a field of 5 T in the same apparatus (see ESI).

Ligand field calculations

LnMo16 series. The four magnetic susceptibility data of the Tb3+, Dy3+, Ho3+ and Er3+ polyanions were used to carry out a simultaneous fit of an effective ligand field hamiltonian. This was based on the Radial Effective Charge (REC) model, which uses effective point charges to model the ligand effects and thus estimate the crystal field parameters in mononuclear lanthanoid complexes (see details in ESI, section 7).57 For this purpose we employed the SIMPRE package, a freely available fortran77 code.58,59 This procedure provided the two parameters, namely the radial displacement and the effective charge, that can be used to describe the ligand field effects of the eight chemically equivalent oxygens of the polyoxomolybdate ligands. As a verification, the magnetic susceptibility of the two remaining members of the series (Tm3+ and Yb3+) was predicted using the same parameters.
LnMo10 series. At the time of our first contact with this family, we had not yet investigated the LnMo16 derivatives with the REC model, and thus we performed an initial (predictive) estimation to evaluate the likelihood of obtaining SMM behaviour in some of the derivatives of this series. For this purpose, we introduced the crystal structures of the Tb3+, Ho3+ and Er3+ derivatives as input in SIMPRE, applying the two REC parameters (radial displacement: Dr = 0.895 Å and effective charge: Zi = 0.105) that had been determined for LnW10 and LnW22 in a previous work.45 On a second stage, we used the product of the radial displacement and the effective charge parameters obtained in the study of the series LnMo16 (f = Dr·Zi = 0.18216) in order to fit the magnetic data of the series LnMo10 while keeping constant f, allowing only one free parameter per compound.

Acknowledgements

The present work has been funded by the EU (ERC Consolidator Grant DECRESIM, COST Actions CM1203 “Polyoxometalate Chemistry for Molecular Nanoscience, PoCheMon” and CA15128 Molecular Spintronics (MOLSPIN)), the Spanish MINECO (grant MAT2014-56143-R, CTQ2014-52758-P and Excellence Unit María de Maeztu MDM-2015-0538 granted to ICMol), and the Generalitat Valenciana (Prometeo Programme of Excellence). A. G.-A. acknowledges funding by the MINECO (Ramón y Cajal contract). E. C. and J. J. B. acknowledge the Blaise Pascal International Chair for financial support. S. C.-S. acknowledges the Generalitat Valenciana for a VALi+D postdoctoral grant. We thank J. M. Martínez-Agudo for performing the magnetic measurements.

Notes and references

  1. S. A. Wolf, D. D. Awschalom, R. A. Buhrman, J. M. Daughton, S. Von Molnár, M. L. Roukes, A. Y. Chtchelkanova and D. M. Treger, Science, 2001, 294, 1488–1495 CrossRef CAS PubMed.
  2. M. E. Flatté, Nature, 2009, 462, 419–420 CrossRef PubMed.
  3. J. Akerman, Science, 2005, 308, 508–510 CrossRef CAS PubMed.
  4. I. L. Prejbeanu, M. Kerekes, R. C. Sousa, H. Sibuet, O. Redon, B. Dieny and J. P. Nozières, J. Phys.: Condens. Matter, 2007, 19, 165218 CrossRef.
  5. B. Georges, J. Grollier, M. Darques, V. Cros, C. Deranlot, B. Marcilhac, G. Faini and a. Fert, Phys. Rev. Lett., 2008, 101, 4–7 CrossRef PubMed.
  6. J. R. Petta, A. C. A. Johnson, J. Taylor, E. A. Laird, A. Yacoby, M. D. Lukin, C. M. Marcus, M. Hanson and A. Gossard, Science, 2005, 309, 2180–2184 CrossRef CAS PubMed.
  7. J. F. Gregg, Nat. Mater., 2007, 6, 798–799 CrossRef CAS PubMed.
  8. K. L. Wang, I. Ovchinnikov, F. Xiu, A. Khitun and M. Bao, J. Nanosci. Nanotechnol., 2011, 11, 306–313 CrossRef CAS PubMed.
  9. A. R. Rocha, V. M. García-Suárez, S. W. Bailey, C. J. Lambert, J. Ferrer and S. Sanvito, Nat. Mater., 2005, 4, 335–339 CrossRef CAS PubMed.
  10. S. Sanvito, Nat. Phys., 2010, 6, 562–564 CrossRef CAS.
  11. J. Camarero and E. Coronado, J. Mater. Chem., 2009, 19, 1678–1684 RSC.
  12. F. Prins, M. Monrabal-Capilla, E. A. Osorio, E. Coronado and H. S. J. Van Der Zant, Adv. Mater., 2011, 23, 1545–1549 CrossRef CAS PubMed.
  13. J. Dugay, M. Giménez-Marqués, T. Kozlova, H. W. Zandbergen, E. Coronado and H. S. J. Van Der Zant, Adv. Mater., 2015, 27, 1288–1293 CrossRef CAS PubMed.
  14. A. Holovchenko, J. Dugay, M. Giménez-Marqués, R. Torres-Cavanillas, E. Coronado and H. S. J. van der Zant, Adv. Mater., 2016 DOI:10.1002/adma.201600890.
  15. R. Sessoli, H. L. Tsai, A. R. Schake, S. Wang, J. B. Vincent, K. Folting, D. Gatteschi, G. Christou and D. N. Hendrickson, J. Am. Chem. Soc., 1993, 115, 1804–1816 CrossRef CAS.
  16. L. Bogani and W. Wernsdorfer, Nat. Mater., 2008, 7, 179–186 CrossRef CAS PubMed.
  17. W. Wernsdorfer, Int. J. Nanotechnol., 2010, 7, 497–522 CrossRef CAS.
  18. E. Cremades, C. D. Pemmaraju, S. Sanvito and E. Ruiz, Nanoscale, 2013, 5, 4751–4757 RSC.
  19. L. Thomas, F. Lionti, R. Ballou, D. Gatteschi, R. Sessoli and B. Barbara, Nature, 1996, 383, 145–147 CrossRef CAS.
  20. C. Paulsen, J.-G. Park, B. Barbara, R. Sessoli and A. Caneschi, J. Magn. Magn. Mater., 1995, 140–144, 1891–1892 CrossRef CAS.
  21. A. Ardavan and S. J. Blundell, J. Mater. Chem., 2009, 19, 1754–1760 RSC.
  22. F. Troiani and M. Affronte, Chem. Soc. Rev., 2011, 40, 3119–3129 RSC.
  23. P. C. E. Stamp and A. Gaita-Ariño, J. Mater. Chem., 2008, 19, 1718–1730 RSC.
  24. J. Lehmann, A. Gaita-Arino, E. Coronado and D. Loss, Nat. Nanotechnol., 2007, 2, 312–317 CrossRef CAS PubMed.
  25. D. N. Woodruff, R. E. P. Winpenny and R. A. Layfield, Chem. Rev., 2013, 113, 5110–5148 CrossRef CAS PubMed.
  26. S. T. Liddle and J. van Slageren, Chem. Soc. Rev., 2015, 44, 6655–6669 RSC.
  27. N. Ishikawa, M. Sugita, T. Ishikawa, S. Y. Koshihara and Y. Kaizu, J. Am. Chem. Soc., 2003, 125, 8694–8695 CrossRef CAS PubMed.
  28. M. Urdampilleta, S. Klyatskaya, J.-P. Cleuziou, M. Ruben and W. Wernsdorfer, Nat. Mater., 2011, 10, 502–506 CrossRef CAS PubMed.
  29. M. Urdampilleta, S. Klayatskaya, M. Ruben and W. Wernsdorfer, ACS Nano, 2015, 9, 4458–4464 CrossRef CAS PubMed.
  30. S. Thiele, F. Balestro, R. Ballou, S. Klyatskaya, M. Ruben and W. Wernsdorfer, Science, 2014, 344, 1135–1138 CrossRef CAS PubMed.
  31. C. Wäckerlin, F. Donati, A. Singha, R. Baltic, S. Rusponi, K. Diller, F. Patthey, M. Pivetta, Y. Lan, S. Klyatskaya, M. Ruben, H. Brune and J. Dreiser, Adv. Mater., 2016, 28, 5195–5199 CrossRef PubMed.
  32. A. Bedoya-Pinto, H. Prima-García, F. Casanova, E. Coronado and L. E. Hueso, Adv. Electron. Mater., 2015, 1500065 CrossRef.
  33. J. J. Baldoví, S. Cardona-Serra, J. M. Clemente Juan, L. Escalera-Moreno, A. Gaita-Ariño and G. Mínguez Espallargas, Europhys. Lett., 2015, 110, 33001 CrossRef.
  34. J. M. Clemente-Juan, E. Coronado and A. Gaita-Ariño, Chem. Soc. Rev., 2012, 41, 7464–7478 RSC.
  35. N. V. Izarova and P. Kögerler, Polyoxometalate-based single-molecule magnets, Trends in Polyoxometalates Research, 2015 Search PubMed.
  36. M. Vonci and C. Boskovic, Aust. J. Chem., 2014, 44, 6655–6669 Search PubMed.
  37. M. Shiddiq, D. Komijani, Y. Duan, A. Gaita-Ariño, E. Coronado and S. Hill, Nature, 2016, 531, 348–351 CrossRef CAS PubMed.
  38. J. J. Baldoví, S. Cardona-Serra, J. M. Clemente-Juan, E. Coronado, A. Gaita-Ariño and H. Prima-García, Chem. Commun., 2013, 49, 8922–8924 RSC.
  39. S. Cardona-Serra, J. M. Clemente-Juan, E. Coronado, A. Gaita-Ariño, A. Camón, M. Evangelisti, F. Luis, M. J. Martínez-Pérez and J. Sesé, J. Am. Chem. Soc., 2012, 134, 14982–14990 CrossRef CAS PubMed.
  40. S. Sherif, G. Rubio-Bollinger, E. Pinilla-Cienfuegos, E. Coronado, J. C. Cuevas and N. Agraït, Nanotechnology, 2015, 26, 291001 CrossRef PubMed.
  41. A. Kitamura, T. Ozeki and A. Yagasaki, Inorg. Chem., 1997, 36, 4275–4279 CrossRef CAS.
  42. C. Bustos, D. M.-L. Carey, K. Boubekeur, R. Thouvenot, A. Proust and P. Gouzerh, Inorg. Chim. Acta, 2010, 363, 4262–4268 CrossRef CAS.
  43. R. Villanneau, A. Proust, F. Robert and P. Gouzerh, Chem. – Eur. J., 2003, 9, 1982–1990 CrossRef CAS PubMed.
  44. R. Villanneau, A. Proust, F. Robert and P. Gouzerh, J. Chem. Soc., Dalt. Trans., 1999, 421–426 RSC.
  45. J. J. Baldoví, J. M. Clemente Juan, E. Coronado, Y. Duan, A. Gaita-Ariño and C. Giménez-Saiz, Inorg. Chem., 2014, 53, 9976–9980 CrossRef PubMed.
  46. J. J. Baldoví, A. Gaita-Ariño and E. Coronado, Dalton Trans., 2015, 44, 12535–12538 RSC.
  47. K. Qian, J. J. Baldoví, S.-D. Jiang, A. Gaita-Ariño, Y.-Q. Zhang, J. Overgaard, B.-W. Wang, E. Coronado and S. Gao, Chem. Sci., 2015, 6, 4587–4593 RSC.
  48. J. J. Baldoví, Y. Duan, R. Morales, A. Gaita-Ariño, E. Ruiz and E. Coronado, Chem. – Eur. J., 2016 DOI:10.1002/chem.201601741.
  49. K. R. Meihaus and J. R. Long, J. Am. Chem. Soc., 2013, 135, 17952–17957 CrossRef CAS PubMed.
  50. S. K. Singh, T. Gupta and G. Rajaraman, Inorg. Chem., 2014, 53, 10835–10845 CrossRef CAS PubMed.
  51. S. Cardona-Serra, J. M. Clemente-Juan, A. Gaita-Ariño, N. Suaud, O. Svoboda and E. Coronado, Chem. Commun., 2013, 49, 9621–9623 RSC.
  52. S. Cardona-Serra, J. M. Clemente-Juan, E. Coronado, A. Gaita-Ariño, N. Suaud, O. Svoboda, R. Bastardis, N. Guihéry and J. J. Palacios, Chem. – Eur. J., 2015, 21, 763–769 CrossRef CAS PubMed.
  53. C. Bosch-Serrano, J. M. Clemente-Juan, E. Coronado, A. Gaita-Ariño, A. Palii and B. Tsukerblat, ChemPhysChem, 2012, 13, 2662–2665 CrossRef CAS PubMed.
  54. C. Bosch-Serrano, J. M. Clemente-Juan, E. Coronado, A. Gaita-Ariño, A. Palii and B. Tsukerblat, Phys. Rev. B: Condens. Matter Mater. Phys., 2012, 86, 024432 CrossRef.
  55. W. Klemperer, Inorg. Synth., 2007, 27, 74–85 CrossRef.
  56. C. Bustos, B. Hasenknopf, R. Thouvenot, J. Vaissermann, A. Proust and P. Gouzerh, Eur. J. Inorg. Chem., 2003, 15, 2757–2766 CrossRef.
  57. J. J. Baldoví, J. J. Borrás-Almenar, J. M. Clemente-Juan, E. Coronado and A. Gaita-Ariño, Dalton Trans., 2012, 41, 13705 RSC.
  58. J. J. Baldoví, S. Cardona-Serra, J. M. Clemente-Juan, E. Coronado, A. Gaita-Ariño and A. Palii, J. Comput. Chem., 2013, 34, 1961–1967 CrossRef.
  59. J. J. Baldoví, J. M. Clemente-Juan, E. Coronado, A. Gaita-Ariño and A. Palii, J. Comput. Chem., 2014, 35, 1930–1934 CrossRef PubMed.

Footnotes

Electronic supplementary information (ESI) available: Elemental analysis results; IR spectra; crystal structure determination details; magnetic properties. CCDC 1446092–1446097 (for LnMo16) and 1482838–1482842 (for LnMo10). For ESI and crystallographic data in CIF or other electronic format see DOI: 10.1039/c6dt02258h
Both authors contributed equally.

This journal is © The Royal Society of Chemistry 2016