Stefania
Tanase
*ab,
Marjo C.
Mittelmeijer-Hazeleger
a,
Gadi
Rothenberg
*a,
Corine
Mathonière
c,
Véronique
Jubera
c,
Jan M. M.
Smits
d and
René
de Gelder
d
aVan't Hoff Institute for Molecular Sciences, University of Amsterdam, Science Park 904, 1098 XH, Amsterdam, The Netherlands. E-mail: s.grecea@uva.nl; g.rothenberg@uva.nl
bLeiden Institute of Chemistry, Gorlaeus Laboratories, Leiden University, PO Box 9502, 2300 RA, Leiden, The Netherlands
cCNRS, Université de Bordeaux, ICMCB, 87 av. Dr A. Schweitzer, Pessac, F-33608, France
dRadboud University Nijmegen, Institute for Molecules and Materials, Toernooiveld 1, 6525 ED, Nijmegen, The Netherlands
First published on 26th August 2011
We report a building blocks approach providing a direct route to multifunctional MOFs, that display photoluminescent properties, robustness, porosity and in some cases unique magnetic properties. The self-assembly of [Mo(CN)8]4− with several in situ prepared lanthanide building blocks gives 3D robust porous networks with open channels. This approach solves the coordination problem, allowing exact placement of the lanthanide ions within the structure. Our MOFs feature good thermal stability and permanent porosity thanks to the strong carboxylate and cyanide linkages. The fact that we have both nitrogen-containing ligand and a π-system means that these MOFs can be excited using low-energy photons. Efficient visible emission was observed for MOFs containing Eu(III) and Tb(III). Surprisingly, the Tb-MOF shows ferromagnetic behavior, proving that the magnetic interaction between Tb(III) ions is strong enough to compensate the ligand field effects.
One of the most exciting applications of MOFs lies in the field of luminescent sensors.14,15 They can be used as analytical sensors or as barcode systems for biological applications.14–16 Constructing such sensor MOFs typically involves assembling lanthanide ions through multifunctional bridging ligands.14,15 However, lanthanides have large coordination spheres and flexible coordination geometries, so inserting them into highly ordered structures is no easy task. One way of overcoming this drawback is by associating the lanthanide ions with transition metal ions.17–20 The problem is that in such a one-pot approach, we cannot control the lanthanide position in the MOF structure. This is a crucial point, because the positioning of the luminescent ion ultimately determines the optical properties. Furthermore, research on lanthanide MOFs is mainly focused on magnetic and photoluminescent properties.14,15 Most lanthanide MOFs lack porosity and therefore their possible applications in gas storage is less explored.
To solve this problem, we present here an elegant synthetic approach for making multifunctional MOFs. We use the affinity of lanthanide ions towards ligands containing hybrid oxygen-nitrogen donors, making in situ lanthanide building-blocks. Then, we assemble these together with [Mo(CN)8]4−, obtaining the desired MOFs. This gives robust hybrid 3D porous networks, with interesting luminescent and magnetic properties.
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Ln-MOF | Isolated Yield (%) |
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Surface Area (m2 g−1) | χMTb (cm−3 K mol−1) |
---|---|---|---|---|
a [Ln(mpca)2(CH3OH)2Ln(H2O)6Mo(CN)8]·8H2O (where Ln = Nd, Eu, Gd, Tb, Er). b χM is the paramagnetic susceptibility measured at T = 300 K. Values in brackets are calculated based on the free ion approximation. | ||||
Nd | 80 | 2122 | 205 | 3.25 (3.28) |
2105 | ||||
Eu | 87 | 2122 | 169 | 3.15 (3.20) |
2105 | ||||
Gd | 85 | 2124 | 179 | 15.47 (15.76) |
2105 | ||||
Tb | 82 | 2125 | n.d. | 29.76 (23.50) |
2104 | ||||
Er | 78 | 2125 | n.d. | 22.72 (22.96) |
2104 |
The IR spectra of Ln-MOFs are basically identical (Figure S1), in agreement with the fact that all MOFs have identical three dimensional structures. The most noticeable feature of the IR spectra concerns the existence of bands at ca. 2122 and 2105 cm−1, which are assigned to the characteristic C≡N stretching vibrations. The very strong peak at 2122 cm−1 confirms the predominant existence of the bridging cyanide groups, indicating the formation of Ln-NC-Mo bridges. All spectra show the presence of the
COO− stretching vibrations around 1605 and 1490 cm−1, thus confirming the presence of the carboxylate groups of the organic ligand. These bands appear as medium to strong absorptions which are shifted to lower frequencies as compared with the free 2-methylpyrazine carboxylic acid. As for the pyrazine ring, the
C≡N stretching frequencies undergo a shift from 1395 cm−1 for the free ligand to ca. 1575 cm−1 upon coordination. These shifts are due to strong coordination of the ring nitrogens with the lanthanide ions, supporting their assignment as chelating ligands.
The absorption spectra collected in the range 200–1400 nm at room temperature of Nd-, Eu- and Er-MOFs as well as of the compound K4[Mo(CN)8] are shown in Figure S4 in the ESI†. The absorption properties bellow 450 nm are ascribed to the π–π* transitions within the ligand and the charge transfer transitions of [Mo(CN)8]4−. In the absorption spectrum of Eu-MOF, the charge transfer transitions of [Mo(CN)8]4− are shifted toward lower energies as compared with the other Ln(III)–Mo(IV) compounds. The EuIII 4f–4f transition lines expected at around 394 nm and 465 nm cannot be distinguished from the large UV absorption band. Eu-MOF is also interesting. The band at 450 nm suggests a peculiar charge transfer which is not observed in the other MOFs. We assign this band to the Eu(III) to Mo(IV) charge transfer. The absorption spectrum of Nd-MOF is rich in bands in the visible and near infrared region. These bands are caused by the transitions from the ground 4I9/2 level to the excited J levels of 4f3 configuration of Nd(III). The excited levels of the visible and near ultraviolet bands are primarily determined by interelectronic repulsion parameters and to a smaller extent by the spin–orbit coupling. The levels producing bands in the infrared being essentially the members of the ground term are separated by multiples. The observed peaks for Nd-MOF correspond to the following transitions: 590 nm (4I9/2 → 4G5/2, 2G7/2); 688 nm (4I9/2 → 4F9/2); 752 nm (4I9/2 → 4F7/2, 4S3/2); 805 nm (4I9/2 → 2H9/2, 4F5/2); 892 nm (4I9/2 → 4F3/2). While Nd(III) has a 4f3 configuration, Er(III) is three electrons shy of the 4f14 configuration. The terms are therefore the same, with and inversion of the order of multiplets. The various levels are more separated in Er-MOF than for Nd-MOF. The ground state of Er(III) is 4I15/2. The observed absorption peaks for Er-MOF correspond to the following transitions: 527 nm (4I15/2 → 2H11/2); 662 nm (4I15/2 → 4F9/2); 811 nm (4I15/2 → 4I9/2); 998 nm (4I15/2 → 4I11/2).
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Fig. 1 The connection between Eu(III) and Mo(IV) in Eu-MOF (top), the connection via the Eu(III) of the 2D planes (middle) and the resulting three-dimensional structure (bottom). Color code: green, europium; yellow, molybdenum; red, oxygen; blue, nitrogen; grey, carbon. Hydrogen atoms and the non-coordinated solvent molecules are omitted for clarity. |
EuMOF | |
---|---|
Formula Weight | 1184.58 |
Crystal System | Monoclinic |
Space Group | P21/c |
a/Å | 10.8137(13) |
b/Å | 19.040(2) |
c/Å | 19.246(4) |
α (°) | 90 |
β (°) | 98.338(11) |
γ (°) | 90 |
V/Å3 | 3920.8(10) |
Z | 4 |
Dcalc (Mg m−3) | 2.0075 |
μ (MoKα) (mm−1) | 3.561 |
Crystal size/mm | 0.23 × 0.13 × 0.11 |
T/K | 208(2) |
Data Collected | 57131 |
Unique data | 8650 |
R int | 0.0276 |
R(F) [I > 2σ(I)] | 7236 |
R w (F2) | 0.0378 |
S | 1.219 |
Δρmin, Δρmax/e Å−3 | −1.535, 1.250 |
Bond lengths | |
---|---|
Eu(1)–O(19) | 2.42 |
Eu(1)–O(29) | 2.40 |
Eu(1)–O(41) | 2.45 |
Eu(1)–O(43) | 2.50 |
Eu(1)–N(10) | 2.62 |
Eu(1)–N(20) | 2.62 |
Eu(1)–N(31) | 2.48 |
Eu(1)–N(32) | 2.46 |
Eu(1)–N(33) | 2.44 |
Eu(2)–O(18) | 2.42 |
Eu(2)–O(51) | 2.42 |
Eu(2)–O(52) | 2.46 |
Eu(2)–O(53) | 2.39 |
Eu(2)–O(54) | 2.35 |
Eu(2)–O(55) | 2.45 |
Eu(2)–O(56) | 2.34 |
Eu(2)–O(28)b | 2.32 |
Mo(1)–C(31) | 2.13 |
Mo(1)–C(34) | 2.15 |
Mo(1)–C(35) | 2.14 |
Mo(1)–C(36) | 2.16 |
Mo(1)–C(37) | 2.15 |
Mo(1)–C(38) | 2.17 |
Bond angles | |
O(19)–Eu(1)–O(29) | 136.34 |
O(19)–Eu(1)–O(41) | 70.02 |
O(19)–Eu(1)–O(43) | 69.37 |
O(29)–Eu(1)–O(41) | 136.26 |
O(43)–Eu(1)–N(32) | 140.92 |
O(43)–Eu(1)–N(33) | 77.07 |
N(10)–Eu(1)–N(20) | 139.06 |
O(18)–Eu(2)–O(51) | 125.69 |
O(18)–Eu(2)–O(52) | 72.62 |
O(18)–Eu(2)–O(53) | 72.33 |
O(51)–Eu(2)–O(54) | 78.15 |
O(51)–Eu(2)–O(55) | 70.26 |
O(51)–Eu(2)–O(56) | 69.71 |
C(31)–Mo(1)–C(36) | 72.78 |
C(31)–Mo(1)–C(37) | 134.60 |
C(31)–Mo(1)–C(38) | 123.29 |
C(35)–Mo(1)–C(37) | 72.51 |
C(35)–Mo(1)–C(38) | 145.72 |
The most remarkable structural feature is the connection of the 2D networks through a second europium(III) center, Eu2. This connection occurs via the carboxylato group of one mpca ligand, giving a 3D structure with open channels (Fig. 1, bottom). Within these channels, voids of 128 Å3 do exist; the shortest H-H distance is about 2.5 Å. The Eu2 center is nine-coordinated. It binds to two bidentate anionic mpca ligands, three cyanide ions, one water molecule and one methanol molecule (Fig. 1, middle). Bond lengths of Eu2–O range from 2.329(2)–2.461(2) Å. The coordination geometry around Eu2 is a slightly distorted square antiprism, with a twist angle of 46.76°. It is the europium-carboxylate bonds that strengthen the 3D structure. Their energy is comparatively large due to enhanced electrostatic attraction. Moreover, the size of the carboxylate functionality allows both bridging and chelation of Eu(III) ions. The structure is further stabilized by multiple hydrogen-bonding between water, methanol and the cyanido ligands.
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Fig. 2 TGA curve of Eu-MOF (top) and the CO2 isotherms of Nd-, Eu- and Gd-MOFs at 273 K (bottom). |
Curiously, Nd-MOF is also a rare example of a coordination network that shows pronounced hysteresis behaviour upon sorption-desorption of CO2, thanks to the structural flexibility of the [Mo(CN)8]4− units. This reflects a dynamic behaviour. Adsorbing CO2, the framework expands to accommodate more guest molecules. When all the CO2 molecules are desorbed, the structure returns to its initial state.
As the lowest excited states of Gd(III) are located at higher energy than the lowest energy excited states of the ligand, no emission is expected for Gd-MOF. Nd(III) and Er(III) are infrared emitting ions whereas Eu(III) and Tb(III) present radiative transitions in the visible range. To detect whether the lanthanide ion can be sensitized by the ligand, we studied the emissive properties of Nd-, Eu-, Tb- and Er-MOFs upon excitation with UV light at 383 nm. This wavelength corresponds to absorption from the ground state to the lowest singlet level of the ligand (see Supplementary Information, Figure S1).21,24
Nd-MOF showed emission at the usual wavelength of 1060 nm, assigned to the 4F3/2 → 4I11/2 transition of Nd(III). Unfortunately, no emission was observed for Er-MOF. The emission spectra of Eu- and Tb-MOFs principally arise from transitions originating at 5D0 and 5D4 levels, respectively (Fig. 3). The spectrum of Eu-MOF shows a weak broad band in the 5D0 → 7F1 transition region. The hypersensitive transition, 5D0 → 7F2, gives the more intense lines with a shoulder at lower frequency (Fig. 1). The resolution of the acquisition is not sufficient to detect the splitting of the 5D0 → 7FJ (J = 3, 4) transitions at room temperature. This lack of precision can also be related to a non-well crystallized environment around the lanthanide ion. The emission spectrum of Tb-MOF shows all the transitions from the emitting 5D4 level to the ground-state manifold. The maximum of the emission is located in the green range of the electromagnetic spectrum; it is due to 5D4 → 7F5 transitions.
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Fig. 3 Emission spectra of Eu-MOF (red) and Tb-MOF (green) at λex = 383 nm. |
The lifetimes were calculated for all the luminescent compositions at the maximum of the emission. Nd-, Eu- and Tb- MOFs have values equal to 91 ns, 1 ms and 1 ms, respectively. These values are shorter than those generally observed in inorganic materials. In coordination compounds, the weak vibronic coupling between lanthanide ions and coordinated water molecules facilitates the non-radiative deactivation.25 This is particularly visible for the Nd-MOF. The lifetimes obtained for Eu- and Tb-MOFs are slightly shorter than those observed for compounds involving organic ligands with similar excited triplet state levels (de-excitation process involving the excited triplet state of the ligands).26,27 This reflects the direct coordination of water molecules to the Eu(III) and Tb(III) ions.
With this in mind, we studied the temperature-dependent magnetic susceptibilities of all MOFs (Fig. 4, top). Note that our MOFs contain a diamagnetic Mo(IV) ion and paramagnetic lanthanide ions connected through carboxylate bridges. Interestingly, the magnetic properties of Nd-, Eu-, and Er- MOFs are indeed dominated by the presence of strong ligand field effects, but Tb-MOF is different. Gd-MOF is of particular interest due the presence of the isotropic Gd(III) ions. These enable an easy interpretation of the magnetic properties with no complications due to the spin–orbit coupling. Starting at room temperature, the χMT values of Gd-MOF are constant down to 10 K. They then decrease slightly to 14.76 cm3Kmol−1 at 1.8 K. The global feature is characteristic of almost no magnetic interactions. A Curie–Weiss fit between 1.8 and 300 K gave the parameters C = 15.35 cm3Kmol−1 and θ = −1.2 K. This result is supported by the reduced molar magnetization at 2 K (Fig. 4b). The saturation magnetization value at 5 T is close to 14 Nβ, and the experimental data show only small deviation from the Brillouin curve (Fig. 5).30
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Fig. 4 Temperature dependence of the χMT products for all MOFs (top). Field dependence of the magnetization recorded at 2 K for Gd- (blue circles) and Tb- (violet circles) MOFs (bottom). |
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Fig. 5 Field dependence of the magnetization recorded at 2 K for Gd-MOF and the corresponding Brillouin curve calculated assuming gGd = 2. Inset: The Curie–Weiss fit between 1.8 and 300 K giving the parameters C = 15.35 cm3Kmol−1 and θ = −1.2 K. |
The terbium-containing MOF is a most peculiar case. Here, the 4f8 ground electronic configuration of Tb(III) yields 7F6 as the ground state and the nearest excited multiplet 7F5 is just little over 2020 cm−1 above. The ligand field splits the 7F6 ground state of Tb(III) in a set of six doublets and one singlet. At lower temperature, the depopulation of these sublevels leads to a deviation from the Curie law. This behavior usually results in a decrease of the χMT product even in the absence of any exchange interaction. But here, surprisingly, when the sample is cooled down from 300 K, the χMT value increases slowly reaching 31.48 cm3Kmol−1 at 27 K. It then decreases slowly to about 31.3 cm3Kmol−1 at 14 K, and increasing again to 32.74 cm3Kmol−1 at 1.8 K. This indicates a ferromagnetic coupling between the two Tb(III) ions, suggesting that the magnetic interaction is strong enough to compensate the ligand field effects. 31,32 Indeed, as shown in the insert of the upper panel in Figure S8 (Supplementary Material), a plot of χ−1versus T in the temperature range below 10 K indicates a positive intercept, characteristic for a ferromagnetic interaction, with a Curie–Weiss temperature of θW ≅ 0.1 K. We have shown previously that the excited levels of the Tb(III) ion are already depopulated below about 10 K.33 The presence of the ferromagnetic interaction between the two Tb(III) ions is also supported by the field dependence of the magnetization at 1.8 K (Fig. 4 bottom) which shows a step increase below 1 T. A subsequent slow and nearly linear increase of magnetization up to 5 T reflects the contributions from the excited levels of the Tb(III) ion. 33 This is supported by the fact that the slope of the linear part yields a susceptibility value about equal to that measured at 100 K.
C, H, and N analyses were performed with a Perkin–Elmer 2400 series II analyzer. Infrared spectra (4000–300 cm−1, resol. 4 cm−1) were recorded on a Perkin–Elmer Paragon 1000 FTIR spectrometer equipped with a Golden Gate ATR device, using the reflectance technique. Diffuse reflectance spectra were obtained on a Perkin–Elmer Lambda 900 spectrophotometer using MgO as a reference. The excitation and emission spectra were recorded with a Perkin Elmer LS50B luminescence spectrometer. The intensity of the emission spectra was corrected for the sensitivity of the detector. Luminescent lifetime was measured using an excimer laser pumped dye laser (Lambda Physik) for excitation (pulse width ∼20 ns) and 0.2 m Acton Research monochromator with a RCA C31034 photomultiplier tube for detection of the emission. Luminescence decay curves were recorded using a Tektronix 200 MHz digital oscilloscope. The TGA was measured using a Setaram TG85 16–18 thermo balance. The heating rate was 5 °C min−1 in helium. The evolved gas was introduced and analysed in a mass spectrometer of Pfeiffer. The CO2 adsorption was performed in a Fisons Sorptomatic 1990. The temperature of the sample was kept constant at 273 K using a Haake DC10 thermostatted bath equipped with a circulating cooler DK15. Temperature dependent magnetic susceptibility and magnetization measurements were performed with a Quantum Design MPMS-5 5T SQUID magnetometer in the temperature range 1.8–300 K and up to 5 T. Samples were embedded in solid icosane to prevent torquing. Data were corrected for the magnetization of the sample holder and for diamagnetic contributions as estimated from the Pascal constants. For Tb-MOF, the temperature dependence of the magnetization was measured in various magnetic fields (0.05, 0.1, 0.2 and 0.5 T). However, no differences in the magnetization curves were observed.
X-ray powder diffraction data were collected on a Philips X'Pert diffractometer, equipped with the X'Celerator, using Cu-Kα radiation. The patterns were measured in the range between 10° and 140° in steps of 0.021 (2°), counting time 10 s.
Footnote |
† Electronic Supplementary Information (ESI) available: IR and optical spectra, XRD and TGA data, decay time curve of Nd-MOF and magnetic properties of Tb-MOF. CCDC reference number 811854. For ESI and crystallographic data in CIF or other electronic format see DOI: 10.1039/c1jm12789f |
This journal is © The Royal Society of Chemistry 2011 |