Aaron J.
Scott
a,
Julia
Vallejo
a,
Arup
Sarkar
b,
Lucy
Smythe
c,
E.
Regincós Martí
c,
Gary S.
Nichol
a,
Wim T.
Klooster
d,
Simon J.
Coles
d,
Mark
Murrie
c,
Gopalan
Rajaraman
*b,
Stergios
Piligkos
*e,
Paul J.
Lusby
*a and
Euan K.
Brechin
*a
aEaStCHEM School of Chemistry, The University of Edinburgh, David Brewster Road, Edinburgh, EH93FJ, UK. E-mail: E.Brechin@ed.ac.uk; Paul.Lusby@ed.ac.uk
bDepartment of Chemistry, Indian Institute of Technology Bombay, Powai, Mumbai 400076, India. E-mail: rajaraman@chem.iitb.ac.in
cWestCHEM, School of Chemistry, University of Glasgow, University Avenue, Glasgow, G12 8QQ, UK
dUK National Crystallographic Service, Chemistry, Faculty of Natural and Environmental Sciences, University of Southampton, England SO17 1BJ, UK
eDepartment of Chemistry, University of Copenhagen, Universitetsparken 5, 2100 Copenhagen, Denmark. E-mail: piligkos@chem.ku.dk
First published on 1st March 2021
Reaction of Ni(OTf)2 with the bisbidentate quaterpyridine ligand L results in the self-assembly of a tetrahedral, paramagnetic cage [NiII4L6]8+. By selectively exchanging the bound triflate from [OTf⊂NiII4L6](OTf)7 (1), we have been able to prepare a series of host–guest complexes that feature an encapsulated paramagnetic tetrahalometallate ion inside this paramagnetic host giving [MIIX4⊂NiII4L6](OTf)6, where MIIX42− = MnCl42− (2), CoCl42− (5), CoBr42− (6), NiCl42− (7), and CuBr42− (8) or [MIIIX4⊂NiII4L6](OTf)7, where MIIIX4− = FeCl4− (3) and FeBr4− (4). Triflate-to-tetrahalometallate exchange occurs in solution and can also be accomplished through single-crystal-to-single-crystal transformations. Host–guest complexes 1–8 all crystallise as homochiral racemates in monoclinic space groups, wherein the four {NiN6} vertexes within a single Ni4L6 unit possess the same Δ or Λ stereochemistry. Magnetic susceptibility and magnetisation data show that the magnetic exchange between metal ions in the host [NiII4] complex, and between the host and the MX4n− guest, are of comparable magnitude and antiferromagnetic in nature. Theoretically derived values for the magnetic exchange are in close agreement with experiment, revealing that large spin densities on the electronegative X-atoms of particular MX4n− guest molecules lead to stronger host–guest magnetic exchange interactions.
Introducing a magnetic guest into the cavity of a magnetic host could result in a number of potential outcomes. (1) Guest encapsulation has no effect, i.e. there is no magnetic interaction between host and guest and/or there is no geometrical change in either component. (2) There is no magnetic interaction between host and guest, but binding induces structural changes, altering the geometries of the metal ions in the cage and/or the encapsulated guest, modifying magnetic anisotropy. (3) There is a magnetic interaction between host and guest, which may or may not also change the magnetic exchange between metals ions in the host. (4) There is a combination of points (2) and (3).
In the chemistry of porous coordination polymers, or metal–organic frameworks (MOFs), the ingress of (non-magnetic) guest molecules into the pores of 3D frameworks built from paramagnetic metal ions, such as CoII, has shown that even simple solvent molecules can modify the magnetic properties of the metal ions via geometry changes induced by intermolecular interactions. The resulting changes in metal anisotropies can lead to significant changes in magnetisation relaxation dynamics.16 In spin crossover (SCO) MOFs the high spin – low spin transition temperature is well known to be highly guest-dependent, proffering potential application in molecular recognition.17,18 Studies of coordination cages and capsules incorporating a paramagnetic component are limited to the examination of magnetic exchange interactions between metal ions in the cage,19 SCO (of the cage and guest),20–23 and the interaction of organic-radicals in the cavity (with themselves or the cage)24–26 or in the host framework.27,28 The ability to understand, and ultimately control, host–guest magnetic exchange interactions and single ion magnetoanisotropies in such molecular species would represent an important step toward making coordination cages with tuneable, and potentially useful, magnetic properties. Herein, we discuss the construction of a tetrahedral cage [NiII4L6]8+ (L = quaterpyridine) that can (reversibly) bind a range of tetrahedral, paramagnetic MX41/2− guests, inducing magnetic exchange interactions between host and guest.
Host–guest complexes 2–8 can also be reversibly formed through single crystal to single crystal transformations. For example, when orange crystals of 1 are soaked in an EtOH solution of (Et4N)2NiCl4 for 2 hours, green crystals of 7 are formed. The process is reversed by soaking crystals of 7 in an EtOH solution of nBu4NOTf (Fig. S1†).
The structures of compounds 1–8 are very similar, and so for the sake of brevity, a generic description is provided. Pertinent bond lengths and angles given in Table S3.† The cationic cage describes a [NiII4L6]8+ tetrahedron, which, akin to other M4L6 assemblies, has the NiII ions occupying the four vertices linked by bisbidentate L ligands lying on each of the six edges (Fig. 1a). The approximate dimensions of the tetrahedron in 1–8 are NiII⋯NiII = 9.2–9.6 Å, with the internal cage volumes ranging from 62–81 Å3. The volumes, pore diameters and average window diameters for each compound are given in Table S4.†30 The NiII ions are six-coordinate and in distorted NiN6 octahedral geometries, with Ni–N distances between 2.03(3)–2.17(3) Å and cis/trans angles in the range 76.4(12)–102.28(13)°/170.3(11)–176.6(6)°, respectively. Each tetrahedron has T-symmetry, possessing four metallic vertices with the same stereochemistry (Δ or Λ). All compounds crystallise as racemic mixtures of the homochiral cage (i.e. an equal mixture of ΔΔΔΔ and ΛΛΛΛ stereoisomers).
Consistent with the ESI-MS observations, 1 has a positionally disordered triflate anion occupying the cavity (Fig. 1b). There are interactions between the O and F atoms of the anion and the inward facing ortho-pyridyl H atoms of L (O/F⋯H−Ar ≈ 2.52 Å). The remaining seven triflate anions surround the exterior of the tetrahedron, maintaining charge balance. These, and the solvent of crystallisation, are involved in a number of intermolecular interactions that connect neighbouring cages.
Complex 7, [NiCl4⊂NiII4L6](OTf)6, is shown in Fig. 2 as a representative tetrahalometallate-cage structure (for depictions of 2–6 and 8, along with pertinent bond lengths and angles, see ESI†). With the exception of 4, which shows a 1:1 partial occupancy of FeBr4− and OTf−, the tetrahalometallate guests are positionally ordered with full occupancy, showing regular tetrahedral geometry. In each case the guest anion is positioned such that the MX4n− tetrahedron is inverted with respect to the cage's [Ni4L6]8+ tetrahedron, i.e. the halide atoms point towards of the portals of the tetrahedron. The host–guest interactions are similar to 1, with the closest contacts between the tetrahalometallate halide atoms and the ortho-pyridyl positions of the cage's ligand. For example, in 7, the distances between the host and guest are: Cl⋯H−Ar ≈ 2.86 Å (Fig. 2b). As with 1, the external triflate anions and solvent of crystallisation connect neighbouring cages through a network of interactions with the host framework. In the extended structure this results in alternating layers of cages/anions and solvent molecules of crystallisation (Fig. S18–S34, Table S5†).
Fig. 2 (a) Portal-view of the [NiCl4⊂NiII4L6]6+ host–guest tetrahedron of 7, illustrating the position of the encapsulated [NiCl4]2−. The tetrahalometallate guest sits with the halide ions pointing towards the cage portals. (b) A close-up of the guest in the host cage highlighting the closest intermolecular interactions (red bonds). Colour code as Fig. 1. Cl = green. |
Fig. 3 χ M T versus T plots for [OTf⊂NiII4L6](OTf)7 (1) and [MIIX4⊂NiII4L6](OTf)6, where MIIX42− = MnCl42− (2), CoCl42− (5), CoBr42− (6), NiCl42− (7), CuBr42− (8) or [MIIIX4⊂NiII4L6](OTf)7, where MIIIX4− = FeCl4− (3), FeBr4− (4) in the range T = 2–300 K and B = 0.1 T. The insets show the field dependence of the magnetisation measured in the T = 2–7 K and B = 0–7.0 T temperature and field ranges. The black spheres are the experimental data and the red lines the fit of the experimental data using spin-Hamiltonian (1), as explained in the text. |
To better define the low temperature magnetic properties of 1–8, we performed variable-temperature-variable-field (VTVB) dc magnetisation measurements on polycrystalline samples in the temperature range 2–7 K and in applied magnetic fields up to 7 T. The results of these VTVB measurements are given in the insets of Fig. 3 as the field dependent magnetisation, and as the magnetisation dependence against the reduced quantity μBB/kT with μB and k the Bohr magneton and Boltzman constant, respectively, (Fig. S35–S42†) that expresses the ratio between Zeeman and thermal energies. Inspection of these reduced magnetisation traces reveals that the ground states of 1–8 are weakly anisotropic, as evidenced by the limited nesting of the curves. Thus, the magnetic anisotropy of the constitutive single ions is either very small, as expected for CuII, FeIII and MnII, or very large (NiII) with respect to the experimental conditions (B, T). For the quantitative interpretation of the magnetic properties of 1–8, we used spin-Hamiltonian (1):
Ĥ = Ĥhost + Ĥguest | (1) |
(2) |
(3) |
The χMT product and the VTVB data for 1–8 were simultaneously fitted to spin-Hamiltonian (1) by full matrix numerical diagonalisation of its matrix representation and by use of the Simplex algorithm.31 For 1, fitting of the χMT product and the VTVB data resulted in the best-fit parameters: gNi = 2.13, |DNi| = 1.575 cm−1 and JNi–Ni = −0.078 cm−1 (Fig. 3). The relatively small uniaxial anisotropy parameter, DNi, of the NiII centres of the host is in agreement with their approximate octahedral symmetry. These parameters were subsequently fixed for the quantitative interpretation of the magnetic properties of 2–8. For simplicity, the g-values of all guests were fixed to 2, except for 7 where we set the g-value of the guest NiII ion equal to gNi = 2.13, as determined for 1. Thus for 2 the model contained only one free parameter, namely JNi–Mn. Simultaneous fitting of the χMT and VTVB data of 2 resulted in the best-fit parameters: JNi–Mn = −0.041 cm−1. Analogously, the best fit parameters for 3 were: JNi–Fe = −0.068 cm−1 (DFe was neglected for FeIII); for 4: JNi–Fe = −0.084 cm−1 (DFe was neglected for FeIII); for 5: |DCo| = 2.37 cm−1 and JNi–Co = −0.005 cm−1; for 6: |DCo| = 6.30 cm−1 and JNi–Co = −0.001 cm−1; for 7: |D′Ni| = 85.5 cm−1 and J′Ni–Ni = −0.476 cm−1; and for 8: JNi–Cu = −0.062 cm−1 (DCu was neglected for CuII). The values are tabulated in Table 1 for convenience. Note that the large D′Ni value for the guest in 7 is of the magnitude expected for a tetrahedral NiII ion, and in agreement with the faster drop of the χMT product with decreasing temperature, absent for all other compounds. For these other compounds, the guest magnetic anisotropy is approximately two orders of magnitude smaller, or entirely negligible.
J (cm−1) | |D| (cm−1) | |
---|---|---|
1 | J Ni–Ni = −0.078 (no MX4 guest – fixed for 2–8) | |DNi| = 1.575 (no MX4 guest – fixed for 2–8) |
2 | J Ni–Mn = −0.041 | Neglected for MnII |
3 | J Ni–Fe = −0.068 | Neglected for FeIII |
4 | J Ni–Fe = −0.084 | Neglected for FeIII |
5 | J Ni–Co = −0.005 | |DCo| = 2.37 |
6 | J Ni–Co = −0.001 | |DCo| = 6.30 |
7 | J′Ni–Ni = −0.476 | |D′Ni| = 85.5 |
8 | J Ni–Cu = −0.062 | Neglected for CuII |
Exp J (cm−1) | Cal J (cm−1) | Exp |D| (cm−1) | Cal D (cm−1) | Exp g-factors/giso | Calc. g-factors/giso/gx, gy, gz | |
---|---|---|---|---|---|---|
1 | J Ni–Ni = −0.078 (no MX4 guest – fixed for 2–8) | J Ni–Ni = −0.062 | 1.575 (fixed for 2–8) | −2.25 (E/D = 0.15) for NiII | 2.13 | g eff = 2.165, 2.171, 2.184 |
2 | J Ni–Mn = −0.041 | J Ni–Mn = −0.011 | Neglected for MnII | −0.002 (E/D = 0.08) for MnII | g eff = 2.00 for Mn | |
J Ni–Ni = −0.078 | J Ni–Ni = −0.090 | |||||
3 | J Ni–Fe = −0.068 | J Ni–Fe = −0.073 | Neglected for FeIII | 0.01 (E/D = 0.26) for FeIII | g eff = 2.00 for Fe | |
J Ni–Ni = −0.078 | J Ni–Ni = −0.074 | |||||
4 | J Ni–Fe = −0.084 | J Ni–Fe = −0.085 | Neglected for FeIII | −0.07 (E/D = 0.16) for FeIII | g eff = 2.00 for Fe | |
J Ni–Ni = −0.078 | J Ni–Ni = −0.073 | |||||
5 | J Ni–Co = −0.005 | J Ni–Co = +0.012 | (Co) 2.37 | −6.64 (E/D = 0.30) for CoII | Co: geff = 1.557, 2.086, 6.619 | |
J Ni–Ni = −0.078 | J Ni–Ni = −0.079 | |||||
6 | J Ni–Co = −0.001 | J Ni–Co = +0.025 | (Co) 6.30 | −3.96 (E/D = 0.17) for CoII | Co: geff = 1.038, 1.234, 6.993 | |
J Ni–Ni = −0.078 | J Ni–Ni = −0.076 | |||||
7 | J′ Ni–Ni = −0.476 | — | (Ni) 85.5 | 213.5 (E/D = 0.26) for NiIItet | Nitet: geff = 3.493, 2.864, 1.689 | |
J Ni–Ni = −0.078 | ||||||
8 | J Ni–Cu = −0.062 | J Ni–Cu = −0.066 | Neglected for CuII | — | (Cu) 2.00 | Cu: giso = 2.43 |
J Ni–Ni = −0.078 | J Ni–Ni = −0.064 |
Fig. 4 Lowest energy broken symmetry spin density plot for complex 2. Iso-surface value, 0.005 e−/Bohr.3 The red and yellow colours represent “spin-up” and “spin-down”, respectively. |
Similar analyses were performed on the remaining host–guest complexes. For complex 3, the JFe–Ni and JNi–Ni interactions are found to be −0.073 cm−1 and −0.074 cm−1, respectively (Table 2). Note that JFe–Ni is stronger than JMn–Ni: a closer examination of the spin densities computed on the Cl atoms of 2 and 3 reveals stronger delocalisation of the spin density in 3 compared to that in 2 facilitating stronger exchange interactions. This is correlated to the shorter Fe–Cl distance (2.20 Å) in 3 compared to the Mn–Cl distance (2.38 Å) in 2. The CASSCF/NEVPT2 computed D values for the guest ions in complexes 2–4 are small. Indeed, they are smaller than the energy separation between the spin state energies arising from the exchange interaction.
A similar situation is observed for complex 4 with [FeBr4]− as the guest. In this case the host–guest antiferromagnetic exchange is larger (−0.085 cm−1) than for 2 and 3. The spin density on the FeIII ion is significantly reduced due to strong spin delocalisation on to the electronegative Cl− and Br− ions in 3 and 4 (Table S6†). Interestingly, in complexes 5 and 6, where [CoCl4]2− and [CoBr4]2− are the guest molecules, JCo–Ni was found to be weakly ferromagnetic from DFT calculations (+0.012 and +0.025 cm−1, respectively; Table 2). The sign of JCo–Ni is contrary to experiment, albeit both the magnitude of the exchange and the absolute difference in the exchange is extremely small. Thus, both experiment and theory point to the presence of extremely weak exchange in this instance, and we note that these particular J values are at the limit of what DFT can accurately reproduce. More importantly, the DCo values determined from ab initio methods are −6.64 cm−1 (5) and −3.96 cm−1 (6), three orders of magnitude higher than the energy separation between the exchange-coupled spin states, i.e., |D| > J. The MS level separations, i.e., the gap between the ±3/2 and ±1/2 microstates for CoII are much larger (∼2|D|) and close to 13 cm−1 and 8 cm−1, respectively. Deviation from ideal Td symmetry is well-known to result in a significant D value for tetrahedral CoII ions.35–38
For complex 7, the orbital degeneracy of the tetrahedral NiII ion precluded convergence of the DFT calculations and thus no host–guest JNi–Ni exchange coupling could be estimated. NEVPT2 calculations yield a D value of +214 cm−1 for [NiCl4]2−, a value much larger than that estimated from experimental susceptibility and magnetisation data.39 The origin of this very large anisotropy can be explained from the NEVPT2-LFT orbital splitting pattern of the pseudo-Td [NiCl4]2− complex shown in Fig. 5. Here the first four excited states contribute strongly to the large positive D value, and arise primarily from the dxy → dyz/dxz and dx2−y2 → dyz/dxz electronic excitations (Table S7†). CASSCF/NEVPT2 calculations carried out on the DFT optimised [NiCl4]2− geometry yield a similar value, D = +210 cm−1. We have also computed the deformation energy of [NiCl4]2− inside the cage. This is calculated as the difference in energy between the DFT optimised structure and the single-point energy calculated on the guest [NiCl4]2−. This is estimated to be 18.6 kJ mol−1, which indicates a small structural distortion upon encapsulation.
In complex 8, the exchange interactions between Ni–Ni and Ni–Cu ions are rather similar, JNi–Ni = −0.064 cm−1 and JNi–Cu = −0.066 cm−1. The spin ground state is S = 1/2 (BS3, Fig. S45†). Due to strong spin delocalisation from the CuII ion onto its four Br− ions the spin density value on the metal ion reduces to just 0.39.
The theoretically determined spin-Hamiltonian parameters have been used to simulate the experimental susceptibility and magnetisation data (Fig. S46–S47†). During simulation, we adopted three different spin-Hamiltonians to describe the magnetic properties for the eight complexes.
For complexes 1–4 and 8 both the metal ions in the host cage and in the guest anions are found to be completely isotropic – the zfs/D values of the MnII, FeIII and NiII(cage) centres are very small and comparable to the J values (i.e. D ≈ J). For these five species, spin-Hamiltonian (4) was employed for simulation. All give very good agreement with the experimental data (Fig. S46†).
For complex 8, the g-factors for the CuII ion from the NEVPT2 level of theory, gx = 1.633, gy = 2.126 and gz = 4.078 are overestimated. This is a well-known problem in the literature for CuII. Higher electron correlation, higher reference space and/or ligand orbital inclusion, should be taken into consideration.40 We have therefore performed multi-reference CI (MRCI) calculations in combination with the CASSCF wavefunction to obtain the final g-factors, gx = 1.945, gy = 2.470 and gz = 2.879 (giso = 2.43), which remain anisotropic due to mixing with the bromide orbitals. Simulation of the susceptibility and magnetisation data shows excellent agreement with the experimental data (Fig. S47†).
(4) |
For complexes 5 and 6, the D parameters of CoII are small but still much larger than the spin state energies/J values (i.e. |D| > J). In these two cases, we have used spin-Hamiltonian (5) to simulate the experimental susceptibility and magnetisation data. Instead of using D values for the CoII ion, ground state effective g-factors for individual Kramers pairs are used as = 1/2 pseudo-spins (Ising Hamiltonian; Table 2).41 This produces a very nice simulation of the experimental data, given the simplicity of the model (Fig. S46–S47†). Note that the simulations are unaffected by the sign of the JNi–Co exchange.
(5) |
(6) |
For complex 7, which contains the highly anisotropic [NiCl4]2− guest anion, we have used spin-Hamiltonian (6) in which all exchange interactions are neglected, since DNi ⋙ J [the inclusion of any reasonable Jhost–guest value does not affect the simulation]. Note that the g-factors obtained from the NEVPT2 method for [NiCl4]2− are overestimated, as expected for the highly anisotropic NiII ion.42 Simulation of susceptibility and magnetisation data is given in Fig. S47† and shows good agreement with the experimental data, albeit of a slightly larger magnitude.
Magnetic susceptibility and magnetisation data show that the magnetic exchange interactions between metal ions in the host complex, and between host and guest, are of comparable magnitude and antiferromagnetic in nature. Theoretically derived values for the exchange are in close agreement with experiment and reveal that large spin densities on the electronegative X-atoms of certain MX4n− guest molecules leads to stronger host–guest magnetic exchange interactions. For the tetrahedral CoII guests, the anisotropy is small but still much larger than the magnitude of exchange coupling between host–host and host–guest. The orbital degeneracy of the tetrahedral NiII ion and the very large zfs that results makes accurate estimation of JNi–Ni and DNi(tet) in (7) rather difficult, as reflected in the large differences in the results obtained between experiment and theory.
What is clear, however, is that the encapsulation of paramagnetic guests inside dia/paramagnetic cages can be very useful in an array of potential applications. These include sensing and switching, the encapsulation and stabilisation of highly anisotropic (and/or air- and moisture-sensitive) magnetic molecules and the organisation (and/or dilution) of magnetic molecules within ordered, solution-stable structural matrices. To date, surface deposition of magnetic molecules has proved problematic, since in the vast majority of cases structural/magnetic integrity is compromised hindering application. Encapsulation of metal complexes such as spin crossover species, single-ion magnets (SIMs) or electron spin based qubits within a dia/paramagnetic cage whose exohedral organic skeleton is easily derivatised may prove to be an interesting option. The cage acting both as a surface anchor and a protective coating for the magnetic molecule.43,44
Although only relatively small changes to the geometries of the MX4n− guests were observed here, this work also suggests that the deliberate distortion/construction of magnetic molecules through encapsulation within the confines of a sterically restricted cavity of a coordination cage may offer an alternative route to producing highly unusual/anisotropic SIMs with specific geometries, tailored ligand fields, and targeted symmetries. In turn, such species may display a breadth of fascinating structures and magnetisation relaxation dynamics that may not exist outwith the cage.
Footnote |
† Electronic supplementary information (ESI) available: Full details of synthetic procedures and characterisation techniques. CCDC 2024429–2024435 and 2023466. For ESI and crystallographic data in CIF or other electronic format see DOI: 10.1039/d1sc00647a |
This journal is © The Royal Society of Chemistry 2021 |