Open Access Article
Sergiu
Shova
a,
Angelica
Vlad
a,
Maria
Cazacu
a,
J.
Krzystek
b,
Andrew
Ozarowski
b,
Michal
Malček
c,
Lukas
Bucinsky
c,
Peter
Rapta
c,
Joan
Cano
d,
Joshua
Telser
*e and
Vladimir B.
Arion
*f
aInorganic Polymers Department, “Petru Poni” Institute of Macromolecular Chemistry, Aleea Gr. Ghica Voda 41 A, Iasi 700487, Romania
bNational High Magnetic Field Laboratory, Florida State University, Tallahassee, Florida 32310, USA
cInstitute of Physical Chemistry and Chemical Physics, Slovak University of Technology in Bratislava, Radlinského 9, 81237 Bratislava, Slovak Republic
dInstitut de Ciència Molecular, Universitat de València, Catedrático José Beltrán Martínez 2, 46980 Paterna, Spain
eDepartment of Biological, Physical and Health Sciences, Roosevelt University, 430 S. Michigan Avenue, Chicago, Illinois 60605, USA. E-mail: jtelser@roosevelt.edu
fInstitute of Inorganic Chemistry of the University of Vienna, Währinger Strasse 42, A1090 Vienna, Austria. E-mail: vladimir.arion@univie.ac.at
First published on 7th January 2019
Three dimanganese(III) complexes have been synthesised and fully characterised by standard spectroscopic methods and spectroelectrochemistry. Each MnIII ion is chelated by a salen type ligand (H2L), but there is variation in the bridging group: LMn(OOCCH
CHCOO)MnL, LMn(OOCC6H4COO)MnL, and LMn(OOCC6H4C6H4COO)MnL. X-ray diffraction revealed an axial compression of each six-coordinate high-spin d4 MnIII ion, which is a Jahn–Teller-active ion. Temperature dependent magnetic susceptibility and variable temperature-variable field (VTVH) magnetisation measurements, as well as high-frequency and -field EPR (HFEPR) spectroscopy were used to accurately describe the magnetic properties of the complexes, not only the single-ion spin Hamiltonian parameters: g-values and zero-field splitting (ZFS) parameters D and E, but also the exchange interaction constant J between the two ions, which has been seldom determined for a di-MnIII complex, particularly when there is more than a single bridging atom. Quantum chemical calculations reproduced well the electronic and geometric structure of these unusual complexes, and, in particular, their electronic absorption spectra along with the spin Hamiltonian and exchange parameters.
Examples of dinuclear complexes with longer manganese-manganese distances are rare in the literature. Of note are the di-MnIII complexes with two salen-type ligands separated by one or two xanthene spacer(s), in which the Mn⋯Mn separation was ∼5.1 Å,26 and with two salicaldehyde/diketonate-derived ligands in which the Mn⋯Mn separation was ∼5.3 Å, and Mn–Mn exchange interactions were observed.27,28 Also notable are di-MnII expanded porphyrins with Mn–Mn distance of 5.4 Å,29 and di-MnII complexes of bis(pentadentate) ligands derived from bis-tacn species with longer Mn⋯Mn distances (≥6.8 Å)30 with no evidence of coupling between paramagnetic centres.
Recently, we reported on the synthesis of mononuclear 3d metal complexes with salen-type ligands bearing a disiloxane moiety (H2L), which were shown to form a central 12-membered chelate cycle when binding to first row transition metal ions, e.g., CuII, FeIII, and MnIII.31–34 In case of manganese, MnIIIL(OAc) and MnIIIL(NCS) were isolated and characterised by single crystal X-ray diffraction, routine spectroscopic methods (UV-vis, IR), spectroelectrochemistry, magnetochemistry, and high-frequency and -field EPR (HFEPR). We show herein that the 12-membered chelate cycle formed by coordination of this unusual salen-type ligand to manganese(III) precludes polymer formation and facilitates the assembly of di-MnIII complexes by using as bridging ligands dicarboxylic acids. Dimanganese(III) complexes with fumarato, terephthalato, and/or p-diphenylcarboxylato bridging ligands were prepared and fully characterised. These complexes are depicted in Fig. 1 and feature Mn⋯Mn distances ranging from 8.7 to 15.1 Å as controlled by the spacer group of the dicarboxylate. Previously reported dimanganese(III,IV) and dimanganese(II,III) systems have been investigated by HFEPR,35–37 and more importantly, so have dimanganese(III) complexes, such as a μ-oxido complex by Retegan et al.,10 a μ-fluorido complex by Pedersen et al.,8 and a system more relevant to those reported here, namely a dimanganese(III,III) complex without any bridging atoms, but with covalent connections between the two MnIII ions via two trans four-bond π-conjugated O–C–C–C–O pathways.28 A tetranuclear complex comprising a square grid of MnIII ions linked by Schiff base ligands has also been studied by HFEPR,38 but this complicated spin system is beyond the present study.
Interestingly, the HFEPR spectra observed here for the dinuclear complexes proved to be of better quality than those reported for the parent mononuclear complex MnIIIL(OAc). We note that the previous HFEPR studies of di-MnIII complexes also exhibited very high quality spectra.8,10,28 These investigations taken together show that a reliable treatment of both the single-ion ZFS interaction and extraction of weak exchange interactions between paramagnetic MnIII (3d4) centres are possible.
CHCOOH), benzene-1,4-dicarboxylic acid (terephthalic acid, C6H4-1,4-(CO2H)2), and biphenyl-4,4′-dicarboxylic acid, 97% (HO2CC6H4C6H4CO2H) were all from Aldrich.
CHCOO)MnL·H2O (1).
A solution of MnL(OAc)·0.15H2O (0.16 g, 0.2 mmol) in methylene chloride (20 ml) in a Schlenk tube was overlayered with a solution of fumaric acid (0.01 g, 0.1 mmol) in dimethylformamide (4 ml). The content was allowed to stand at room temperature. Brown sticks formed within one month and were separated by filtration, washed with diethyl ether and dried at room temperature. Yield: 0.11 g, 69.4%. Anal. Calcd (%) for C84H136Mn2N4O11Si4 (Mr 1645.26): C, 61.32, H, 8.64, N, 3.41. Found: C, 61.31, H, 8.40, N, 3.42. IR spectrum (KBr pellet), selected bands, νmax (cm–1): 3442w, 2956vs, 2868s, 1676vs, 1618vs, 1550s, 1440s, 1355m, 1298m, 1255vs, 1174m, 1066s, 977w, 921w, 885m, 840s, 785s, 746m, 698m, 634w, 565s, 509w, 468vw, 441w. X-ray diffraction quality crystals were grown from a mixture of CH3OH
:
CH2Cl2 (∼3
:
1). ESI-MS (positive ion mode): m/z 733.42 [MnIIIL]+.
:
CH2Cl2 (∼4
:
1). ESI-MS (positive ion mode): m/z 733.42 [MnIIIL]+.
:
methanol 1
:
1 (4 ml) at about 60 °C. The content was allowed to stand at room temperature. Brown sticks formed within one month and were separated by filtration, washed with diethyl ether and dried at room temperature. Yield: 0.02 g, 91.0%. Anal. Calcd (%) for C94H142Mn2N4O11Si4 (Mr 1726.37): C, 65.40, H, 8.29, N, 3.25. Found: C, 65.61, H, 8.19, N, 3.41. IR spectrum (KBr pellet), selected bands, νmax (cm–1): 3437m, 2956vs, 2910s, 2868s, 1676s, 1616vs, 1581m, 1541s, 1436s, 1396vs, 1355m, 1307m, 1253vs, 1174s, 1132w, 1064s, 972w, 921vw, 885m, 842vs, 777s, 694m, 636w, 567m, 509w, 439w. ESI-MS (positive ion mode): m/z 733.42 [MnIIIL]+.
| Compound | 1·6CH2Cl2 | 2·4CH2Cl2 | 3·4.5H2O |
|---|---|---|---|
| a R 1 = Σ| |Fo| − |Fc| |/Σ|Fo|. b wR2 = {Σ[w(Fo2 − Fc2)2]/Σ[w(Fo2)2]}1/2. c GOF = {Σ[w(Fo2 − Fc2)2]/(n − p)}1/2, where n is the number of reflections and p is the total number of parameters refined. | |||
| Empirical formula | C90H146Cl12Mn2N4O10Si4 | C92H144Cl8Mn2N4O10Si4 | C94H151Mn2N4O15.5Si4 |
| F w | 2091.75 | 1971.95 | 1807.43 |
| T [K] | 100 | 100 | 100 |
| Crystal system | Triclinic | Triclinic | Monoclinic |
| Space group |
P![]() |
P![]() |
P21/c |
| a [Å] | 13.7007(7) | 11.8837(17) | 15.790(2) |
| b [Å] | 14.7166(7) | 12.7755(19) | 14.221(2) |
| c [Å] | 15.9617(8) | 18.564(3) | 23.958(3) |
| α [°] | 67.7592(16) | 73.414(5) | |
| β [°] | 66.1603(17) | 81.359(5) | 106.126(5) |
| γ [°] | 79.2085(17) | 72.378(5) | |
| V [Å3] | 2722.5(2) | 2568.1(6) | 5168.3(13) |
| ρ calcd [g cm−3] | 1.276 | 1.275 | 1.161 |
| Z | 1 | 2 | 4 |
| μ [mm−1] | 0.622 | 0.555 | 0.350 |
| Crystal size [mm] | 0.528 × 0.523 × 0.485 | 0.32 × 0.14 × 0.04 | 0.41 × 0.096 × 0.072 |
| 2Θ range | 4.88 to 60.22 | 4.62 to 50.06 | 4.56 to 50.06 |
| Reflections collected | 61 020 |
8962 | 64 669 |
| Independent reflections | 15 855 [Rint = 0.0461] |
8962 [Rint = 0.045] | 9090 [Rint = 0.0576] |
| Data/restraints/parameters | 15 855/6/605 |
8962/0/558 | 9090/3/567 |
| R 1 | 0.0539 | 0.0765 | 0.0779 |
| wR2b | 0.1653 | 0.2270 | 0.2170 |
| GOFc | 1.040 | 1.061 | 1.030 |
| Largest diff. peak/hole/e Å−3 | 1.04/−2.08 | 1.25/−1.15 | 1.88/−0.98 |
Multifrequency HFEPR data obtained for 1 and 2 were fitted using the following spin Hamiltonian:
| H = βeBgŜ + D[Ŝz2 − S(S + 1)/3] + E(Ŝx2 − Ŝy2) | (1) |
(a) Theoretical calculations based on both an ab initio method, namely the Complete Active Space (CAS) multi-configurational method, as well as at the DFT level using the PBE functional,45 on the full MnIIIGaIII dinuclear complexes of 1–3 were performed for determining the MnIII single-ion ZFS. These calculations were carried out using the TZVP basis set proposed by Ahlrichs46–48 and the auxiliary TZV/C Coulomb fitting basis sets.49–51 The second order contributions to ZFS were evaluated for the five quintet and 30 triplet excited states generated from an active space with four electrons in five d orbitals. Furthermore, to estimate the dynamic electron correlation effects on ZFS parameters, mononuclear models built from a truncation of the original molecules were carried out by the CAS method and subsequent second-order N-electron valence state perturbation theory (NEVPT2).52
(b) For the sake of comparison with the previous studies on [MnL(NCS] and [MnL(OAc)],31,33 additional calculations have been performed using the BLYP functional53 and 6-311G*54 basis set using the CASSCF and Multi-Reference Configuration Interaction (MRCI) approaches. These calculations used the crystal structure geometries of 1–3 with the entire second MnIII-containing moiety removed (refer to ESI† for further details). In addition, the effect of the solvent molecules present in the crystal structure has been studied for brevity at the BLYP/6-311G* level. The spin–spin interaction has been accounted via the MRCI55 approach for the state-averaged quintet CASSCF(4,5) wave function.
(c) In addition, the multi-centre (i.e., both MnIIIL moieties and the bridging ligand) CASSCF(8,10) ZFS parameters have been compared to CAS(8,10)-CI results (automatic auxiliary fitting basis set was used) for 1–3. The L-CASCI approach has followed consistently the protocol as described in the literature.56 The L-CASCI calculations accounted both for spin–orbit and spin–spin couplings (SOC and SSC, respectively).
For an additional comparison to spectroelectrochemistry studies, B3LYP53/6-311G*54 geometry optimisations of neutral (nonet), single (octet) and doubly (septet) charged species of 1–3 have been performed using the Gaussian09 software suite.57 Subsequently, electronic transitions of all the B3LYP/6-311G* optimised structures were evaluated using the TD-DFT method.58 Herein, the 40, 60, and 80 lowest excited states were taken into account for the neutral, single and doubly charged species, respectively, to approach transition energies corresponding to λ ≥ 300 nm. Spin densities were visualised using Molekel59 software suite.
To extend further the computations used to assess the EPR parameters in the single-ion models, the possibility of a magnetic exchange interaction between the two MnIII ions was studied at the DFT level of theory. These calculations were performed with the CAM-B3LYP hybrid functional using the Gaussian 09 package,57 the quadratic convergence approach, and a guess function generated with the fragment tool of the same program.53,60 Triple-ζ and double-ζ all-electron basis sets proposed by Ahlrichs et al. were respectively employed for the Mn ions and the remaining atoms.47,48 The magnetic coupling states were obtained from the relative energies of the broken-symmetry (BS) singlet spin state from the high-spin state with parallel local spin moments.61–63 A polarisable continuum model (PCM) was introduced in the calculations with the parameters corresponding to acetonitrile.64 To assure that the precision of the results was higher than the magnitude of the estimated J values, a triple-ζ basis set, adding an extra p polarisation function for all atoms, together with restricted conditions in the self-consistent convergence of the wave-function and in the evaluation of the bi-electronic integrals (very tight and ultrafine, respectively) were also employed.
:
1 afforded single crystals of X-ray diffraction quality.
The analysis of the crystal structure packing revealed that all the compounds are associated in the crystal only through the C–H⋯π interactions to form either supramolecular chains or ribbon-like aggregates. Thus, the crystal structures of 1 and 3 are built up from the parallel packing of one-dimensional chains, as shown in Fig. S1a and S1b (ESI†), respectively. The crystal packing of 3 shows the presence of the supramolecular ribbons (Fig. S2, ESI†).
A small additional peak is seen behind the first one for 1 and 3 which height varies from scan to scan indicating the follow up reactions of the oxidised state (see also Fig. S3a, ESI†). No reduction processes were observed in cathodic region (see Fig. S3b, ESI†) as also noted for MnL(OAc). After electrolysis of 1–3 in the region of the first irreversible oxidation peak, no X-band EPR signal was observed even at 77 K further indicating a low stability of the oxidised form of 1–3. Although a negative EPR result at 77 K is not proof of the inability to electrochemically generate MnIV species in solution, we note that a variety of bona fide MnIV coordination complexes exhibit EPR spectra (even in some cases as magnetically undiluted solids) at temperatures as high as ambient.65–67 However, there are small differences in the voltammetric responses found for 1–3. The highest oxidation potential was found for 2 with only one oxidation peak demonstrating the (electro)chemical equivalence of the two MnIII sites and the lack of measurable interaction between them, consistent with the magnetometry and HFEPR. For 3 the lowest oxidation potential was found with two overlapping oxidation peaks again indicating two almost equal MnIII redox centres.
Analogously to the voltammetric studies, the optical spectra of 1–3 are very similar with low-intensity bands at 480, 670 and at around 730 nm (Fig. 4a).
Taking into account our previous works31,33 on mononuclear MnIIIL(OAc) and MnIIIL(NCS), the first low-energy electronic transition at 730 nm can be assigned to LMCT from phenolate moieties to manganese(III) with a strong charge transfer from phenolic moieties to the central Mn atom and the corresponding coordination polyhedron. The in situ UV-vis-NIR spectroelectrochemical experiments confirmed irreversible changes upon anodic oxidation of 1–3 in the region of the first oxidation peak (from +0.2 V to +0.9 V vs. Fc+/Fc) as illustrated for 2 in Fig. 4b. A new optical band at 360 nm emerged upon oxidation and simultaneously the maximum of the low-energy band shifted from 720 nm to 675 nm (see inset in Fig. 4b). However in contrast to the recently studied MnIIIL(NCS) complex,34 upon scan reversal the products that are formed upon oxidation are not reoxidised and no recovery of the initial optical bands upon the voltammetric reverse scan occurred, confirming the low stability of MnIV state as also reported for the MnIIIL(OAc).31
![]() | ||
| Fig. 5 Plots of χMT vs. T in the range 2–300 K in a 0.025 (T < 20 K) and 0.5 T (T ≥ 20 K) applied field and M vs. H/T (inset) for (a) 1, (b) 2, and (c) 3 in the 2–10 K temperature range. The solid lines are the best-fit curves, with the fit parameters given in Table 2. | ||
![]() | ||
| Fig. 6 Low-temperature HFEPR spectra of 1 at 422.4 GHz and 15 K (top) and 2 and 406.4 GHz and 10 K (bottom, both represented as black traces) accompanied by simulations using S = 2 spin Hamiltonian parameters as in Table 2. Blue traces: simulations using negative D; red traces: positive D. | ||
Complex 2 was visibly more crystalline than 1. This required extensive grinding prior to pressing it into a pellet. A typical low-temperature pellet spectrum is shown in Fig. 6 (bottom), accompanied by simulations assuming a perfect powder distribution of the crystallites in space. Additional spectra at two different frequencies are shown in Fig. S6 and S7, ESI.† The spectral quality was somewhat lower than that for 1 because of the sample crystallinity, yet the agreement between the simulations and experiments can be also described as very good, assuming again an S = 2 spin state, and under the condition of D > 0. The spin Hamiltonian parameters are similar but not identical to those of 1.
Both complexes produced HFEPR spectra at any temperature between liquid helium and ambient. Fig. 7 shows their room-temperature spectra, again with simulations. In complex 1, the axial ZFS parameter D is almost unchanged between liquid helium and room temperature (Table 2), but |E| strongly decreases, the ZFS tensor becoming almost axial. In 2, both parameters slightly decrease from low to high temperature.
![]() | ||
| Fig. 7 Room-temperature HFEPR spectra of 2 at 203.2 GHz and 280 K (top) and 2 at 295.2 GHz and 277 K (bottom, black traces) accompanied by simulations using spin Hamiltonian parameters as in Table 2. At these temperatures, there is no difference between negative and positive D reflected in the spectra, thus the simulation (red trace) used positive D only. The MnII impurity resonances at g = 2.00 were left out of the experimental spectra and are not simulated. | ||
| Complex | T (K) | D (cm−1) | |E| (cm−1) | |E/D| | g x | g y | g z |
|---|---|---|---|---|---|---|---|
| a The magnetic fits used an isotropic g value which is given only in this column. b Compound 3 was investigated only by magnetometry due to material limitations. c The room temperature HFEPR parameters are of lower precision (not specified) and are provided primarily to demonstrate that the electronic structures of 1 and 2 remain essentially unchanged over a wide temperature range. | |||||||
| 1 | 15 | +3.246(5) | 0.425(3) | 0.13 | 1.991(4) | 2.003(4) | 2.015(5) |
| 1 | 280c | 3.27 | 0.10 | 0.03 | 1.98 | 1.98 | 2.00 |
| 1 (magn.) | NA | +3.07 | 0 | 0.000 | — | — | 2.004 |
| 2 | 10 | +2.997(3) | 0.530(1) | 0.18 | 1.991(5) | 1.991(5) | 1.991(5) |
| 2 | 277c | 2.88 | 0.44 | 0.15 | 1.99 | 1.99 | 1.99 |
| 2 (magn.) | NA | +3.45 | 0.03 | 0.009 | — | — | 2.033 |
| 3 (magn.) | NA | +3.63 | 0.007 | 0.002 | — | — | 2.019 |
A careful inspection of certain turning points in the low-T HFEPR spectra of both 1 and 2 reveals spectral regions at any frequency >200 GHz that show a fine but not quite regular structure with a period of ca. 60–80 mT (Fig. 8). The average value of 70 mT corresponds to 0.065 cm−1, which is very small on the HFEPR scale as it corresponds to ∼2 GHz (∼1% of the frequency used in Fig. 8, right), but is still well within spectral resolution present. Yet, this energy is one order of magnitude more than that from 55Mn hyperfine coupling, which could (potentially) be expected to appear in the spectra.70 We postpone a discussion of this observation noting qualitatively that this could be a symptom of a very weak (<0.1 cm−1) exchange taking place between the two MnIII ions in the dimer.
![]() | ||
| Fig. 8 Fragments of HFEPR spectra of 1 at 406.4 GHz and 10 K (left) and 2 at 203.2 GHz and 10 K (right). Blue: Experimental. Red: Calculated using spin Hamiltonian 2 (dimer model, eqn (2)). Green: Calculated using spin Hamiltonian 1 (monomer model, eqn (1)). The indicated splittings appear also in other regions of the spectra, and at different frequencies. | ||
The low-T spin Hamiltonian parameters used in the simulations shown in Fig. 6 were not deduced from the single-frequency spectra, but from the 2-D maps of turning points as a function of frequency/energy according to the principle of tuneable-frequency EPR.72 These maps are shown in Fig. 9. The parameters are listed in Table 2. The room temperature parameters, to the contrary, were obtained from single-frequency spectra only and because of the poor S/N are estimates only.
![]() | ||
| Fig. 9 Field vs. frequency/energy map of turning points in complexes 1 (top) and 2 (bottom) at 10–15 K. Squares are experimental points; curves were simulated using spin Hamiltonian parameters as in Table 2. Red curves: turning points with magnetic field B0 parallel to the x-axis of the ZFS tensor; blue: B0 || y; black: B0 || z. The two dashed vertical lines indicate the frequencies at which spectra shown in Fig. 6 were recorded. | ||
To explore the effect of the interactions between the MnIII ions, the spin Hamiltonian in eqn (1) must be replaced by eqn (2) which operates within the space of 25 microstates in a system of two ions with S1 = S2 = 2:
![]() | (2) |
D (thus D, E are as in eqn (1)) and are coaxial as well.74 In the present case, D12 is most likely due only to the magnetic dipole–dipole interaction, which depends on the crystallographically-determined inter-ion distance R and can be estimated from:![]() | (3) |
The largest component of the dipolar tensor is along the Mn–Mn direction which is almost perpendicular to the expected direction of the largest component of the ZFS tensor on each MnIII ion, which is along the O(phenolato)–Mn–O(phenolato) axis (i.e., the axial compression axis; see discussion below and Fig. S9, ESI†). Eqn (3) results in D12 values of −0.008 cm−1 for 1 and −0.004 cm−1 for 2. These magnitudes should be treated as an upper estimation as delocalisation effects of the MnIII spins are not taken into account, but are even so much too small to account for the observed splitting of at least ∼60 mT. Nevertheless, for completeness, the EPR simulations for both 1 and 2 included these D12 values.
In contrast, for systems with single atom bridges, such as μ-oxido10,11 or -fluorido,8 the crystallographically-determined distances of ∼3.16 Å and 4.10 Å, would give a maximum direct dipole–dipole coupling some 20 times larger: −0.16 cm−1 and −0.075 cm−1, respectively. Even in the phenolato/diketonato-linked complex, the Mn–Mn distance of 5.26 Å would give D12 ≈ −0.036 cm−1.
However, in each of these three complexes previously studied by HFEPR, a direct covalent pathway between the MnIII ions leads to an isotropic exchange interaction (eqn (2)) that overwhelms the dipolar effect. Use of the JS1S2 formalism (as opposed to −2J or other variants) yields J (in cm−1) = −2.3, +33.0(2), and +1.70, as respectively reported for each.8,10,11,28 The linear MnIII-(μ-F)-MnIII leads to a strong antiferromagnetic “bonding-like” interaction, but in the other complexes the anti- or ferromagnetic nature of the exchange coupling is not obvious. As explored by Retegan et al.,10 and others24,75 for di-MnIII, by Morsing et al. for di-CrIII,76 and by Weihe and Güdel for di-FeIII,77 the specific geometry of the M-(μ-O[X])-M moiety (X = none, H, R) has a profound effect on the exchange coupling parameter.
In our systems, wherein the Mn–Mn distances are much greater and the covalent pathways more convoluted, simulations nevertheless show that the isotropic exchange interaction is indeed responsible for the observed spectral effects. The J (and D12, if it were larger) terms split the energy levels of a monomer which results in splitting of the single-ion resonances calculated using eqn (1) each into several components (Fig. 10 and S8, ESI†). Since powder spectra are superpositions of a very large number of single-crystal spectra, these splittings are mostly blurred and are recognisable only in certain magnetic field ranges allowing only a rough estimation of J.
![]() | ||
| Fig. 10 Right: Energy levels of a monomer, calculated at the “z” orientation, using eqn (1) with parameters of 1 (Table 2). Left: Energy levels of a dimer, calculated using eqn (2) with the same single-ion g, D and E parameters of 1 and with J = −0.025 cm−1. The vertical lines represent EPR transitions expected at ν = 406.4 GHz. Only transitions with substantial probability are drawn. Colours are used to distinguish very close transitions. See also Fig. S8, ESI.† | ||
Nevertheless, one can see that in 1, an isotropic exchange term with J = −0.025 cm−1 (ferromagnetic), which is some 100 times smaller than D, is sufficient to split a “z” transition in 1, which in a monomer occurs at 11.16 T, so that the outermost components are 180 mT apart (Fig. 6, 8, 10, and S8, ESI†). Spectra of 2 appear to simulate better with positive J of +0.035 cm−1. It is clear that exchange interactions of such small energy cannot be detected by magnetic measurements, nor would they affect the electrochemistry. The J magnitudes above must be treated as estimations, but single-crystal EPR experiments may provide accurate J values. Interestingly, some of us have recently observed similar effects in HFEPR of very different systems.78 It should also be noted that NMR can be used to probe exchange couplings as shown by the linear correlation between μ-acetato methyl proton chemical shifts and J values that was established for a series of dimanganese(III) complexes containing {Mn2O(μ-O2CCH3)2}2+ cores.22
| Method | |||||||
|---|---|---|---|---|---|---|---|
| Complex | CASa | NEVPT2a | CAS (SOC)b | L-CASCI (SOC)b | MRCI (SOC + SSC)b | L-CASCI (SOC)c | L-CASCI (SOC + SSC)c |
| a Calculated for single-centre geometries from a second order perturbative spin–orbit coupling Hamiltonian applied to the CAS MnGa model and NEVPT2 wavefunctions of the single Mn centre (using TZVP basis set) of model (a). b Calculated for single-centre geometries (using 6-311G* basis set) of model (b). c Calculated for two-centre (using 6-311G* basis set and the autoaux density fitting basis set) using model (c). | |||||||
| 1 | +3.44 (0.234) | +3.57 (0.227) | +2.94 (0.228) | +2.93 (0.227) | +3.64 (0.136) | +2.62 (0.224) | +3.47 (0.234) |
| 2 | +3.55 (0.159) | +3.64 (0.154) | +3.03 (0.154) | +3.03 (0.155) | +3.52 (0.159) | +2.71 (0.151) | +3.58 (0.163) |
| 3 | +3.67 (0.151) | +3.87 (0.147) | +3.14 (0.133) | +3.14 (0.132) | +3.41 (0.232) | +2.81 (0.129) | +3.69 (0.137) |
The obtained results lead to a positive D value (Table 3) which is consistent with the axial (tetragonal) compression observed experimentally in the three complexes (Table 2), but with a significant rhombic distortion, in agreement with HFEPR spectroscopy. This similar axial distortion in 1–3 leads to close D values. However, the trend in the SOC CAS results is also corroborated by DFT calculations (Tables S2 and S3, ESI†), although this method underestimates the D values in manganese(III) complexes.32,34,55b Generally, the SOC CAS results lead to an increase of D parameter with the size of the bridging ligand (see Table 3), which correlates well with the susceptibility fit in Table 2. On the contrary, the inclusion of SSC via MRCI reverses this trend in the single centre calculations of model (b) (see Table 3), which is in accordance with HFEPR (see Table 2) for 1 and 2. HFEPR of powders or solutions does not provide the orientation of the ZFS. However, this can be calculated, and in Fig. S9 (ESI†) are displayed the orientations of the principal axes of the D tensors of 1–3 in the molecular coordinate system obtained in model (a). As expected, the principal z-axis (“hard” axis) points at the oxygen atoms of the coordinated phenolato groups, i.e., along the axis of compression. Lastly, the g-tensors for 1–3 calculated from the NEVPT2 method and using an effective Hamiltonian for the spin–orbit coupling (Table S4, ESI†) agree moderately well with those obtained by HFEPR spectroscopy, with the calculated values being slightly below 2.0 which agrees with the high temperature HFEPR fit in Table 2, and is expected from classical theory for a less than half-filled dn system.
As can be seen from Fig. 11, spin density is localised almost exclusively in the vicinity of the two MnIII ions in the case of the neutral complex 1. Upon oxidation to 1+, part of the spin (about 0.5e) vanishes from these ions (Fig. S10a†). Finally, the doubly charged species, 12+ (septet), has the spin population decreased by one, hence both centres are oxidised to MnIV (Fig. S10b†). The calculated TD-DFT transitions (Fig. 11a) of 1 are in qualitative agreement with the experimental UV-vis spectra (Fig. 4). Comparison of singly and doubly oxidised species with the measured difference spectra are not useful due to irreversible chemical changes of 1–3 upon oxidation.
Finally, CAM-B3LYP DFT calculations on 1–3 showed that the intramolecular magnetic coupling in 1 is ferromagnetic (i.e., J exchange coupling constant is negative: H = JS1S2) and weak, J = −0.007 cm−1, while in 2 and 3 it is antiferromagnetic with J of 0.004 and 0.022 cm−1, respectively. The magnetic communication in an extended pathway can occur only through a π-pathway. A loss of its planarity causes a notable decrease in the aromaticity and the magnetic coupling. In 1–3, the privation of this planarity comes mainly from a twist between the carboxylate groups and the vinyl (in 1: 11.3° twist) or phenyl rings (2: 26.2° and 3: 17.4–20.0°), and between phenyl rings in 3 (≈38°). Neither these structural distortions nor electronic effects such as accidental orthogonality of magnetic orbitals can explain the trend found for the J constants for 1–3. Hence, speculation as to the structural/electronic basis for the opposite type of exchange coupling in 1versus2 and 3 is unwarranted given the very small magnitude of these interactions and the challenges of understanding exchange interactions even in singly bridged systems.10,24,68,75,79 Nevertheless, the DFT results for 1 and 2 are in qualitative agreement with the EPR data.
CHCOO)MnL (1), LMn(OOCC6H4COO)MnL (2), and LMn(OOCC6H4C6H4COO)MnL (3), respectively. The anodic oxidation of these complexes is irreversible and is similar to the monomeric MnL(OAc) analogue. Complex 3 exhibited the lowest oxidation potential with two overlapping oxidation peaks indicating a slightly different oxidation potential for the two MnIII redox centres. By using temperature dependent magnetic susceptibility and variable temperature-variable field (VTVH) magnetisation measurements and high-frequency and -field EPR (HFEPR) spectroscopy, the single-ion spin Hamiltonian parameters (g values, ZFS parameters D and E) were obtained and reproduced successfully by ab initio calculations. The quality of HFEPR spectra of 1 and 2 was superior to that of the analogous mononuclear complex MnL(OAc). This allowed identification of characteristic signatures in high-resolution spectra which presumably indicate very weak exchange interactions between the paramagnetic ions and estimation of the exchange coupling constant, |J| ≈ 0.03(5) cm−1, (JS1S2 formalism) which was in reasonable agreement with DFT calculations for 1 and 2. This result suggests that magnetic exchange interactions can occur in di-MnIII systems over relatively long distances (as much as ∼11 Å), which may be the case in biological di- and multi-Mn systems as well.
Footnote |
| † Electronic supplementary information (ESI) available: Computational details and discussion of theoretically determined EPR properties; packing features of 1, 3 (Fig. S1) and 2 (Fig. S2), cyclic voltammograms of 1 and 2 (Fig. S3), HFEPR spectra of 1 and 2 (Fig. S4–S7), fragment of the experimental HFEPR spectrum of 1 and energy levels of a dimer with and without exchange interaction between MnIII ions (Fig. S8), relative orientations of the experimental coordination sphere geometry of 1–3 and the calculated D tensor (Fig. S9); theoretical spin densities and electronic transitions of 1+ and 12+ (Fig. S10); bond distances and angles 1–3 (Table S1), estimated values of the D and E/D ratio for 1–3 (Tables S2 and S3), calculated g-tensor components for 1–3 (Table S4), L-CASCI reference space used (Table S5). CCDC 1875357–1875359. For ESI and crystallographic data in CIF or other electronic format see DOI: 10.1039/c8dt04596h |
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