Variation of the ground spin state in homo- and hetero-octanuclear copper(ii) and nickel(ii) double-star complexes with a meso-helicate-type metallacryptand core
作者:Emilio Pardo、Marie-Claire Dul、Rodrigue Lescouëzec、Lise-Marie Chamoreau、Yves Journaux、Jorge Pasán、Catalina Ruiz-Pérez、Miguel Julve、Francesc Lloret、Rafael Ruiz-García、Joan Cano
DOI:10.1039/b926709c
日期:——
Homo- and heterometallic octanuclear complexes of formula Na2[Cu2(mpba)3][Cu(Me5dien)]6}(ClO4)6·12H2O (1), Na2[Cu2(Mempba)3][Cu(Me5dien)]6}(ClO4)6·12H2O (2), Na2[Ni2(mpba)3][Cu(Me5dien)]6}(ClO4)6·12H2O (3), Na2[Ni2(Mempba)3][Cu(Me5dien)]6}(ClO4)6·9H2O (4), [Ni2(mpba)3][Ni(dipn)(H2O)]6}(ClO4)4·12.5H2O (5), and [Ni2(Mempba)3][Ni(dipn)(H2O)]6}(ClO4)4·12H2O (6) [mpba = 1,3-phenylenebis(oxamate), Mempba = 4-methyl-1,3-phenylenebis(oxamate), Me5dien = N,N,N′,N′′,N′′-pentamethyldiethylenetriamine, and dipn = dipropylenetriamine] have been synthesized through the “complex-as-ligand/complex-as-metal” strategy. Single-crystal X-ray diffraction analyses of 1, 3, and 5 show cationic MII2M′II6 entities (M, M′ = Cu and Ni) with an overall double-star architecture, which is made up of two oxamato-bridged MIIM′II3 star units connected through three meta-phenylenediamidate bridges between the two central metal atoms leading to a binuclear metallacryptand core of the meso-helicate-type. Dc magnetic susceptibility data for 1–6 in the temperature range 2–300 K have been analyzed through a “dimer-of-tetramers” model [H = −J(S1A·S3A + S1A·S4A + S1A·S5A + S2B·S6B + S2B·S7B + S2B·S8B) −J′S1A·S2B, with S1A = S2B = SM and S3A = S4A = S5A = S6B = S7B = S8B = SM′]. The moderate to strong antiferromagnetic coupling between the MII and M′II ions through the oxamate bridge in 1–6 (−JCu–Cu = 52.0–57.0 cm−1, −JNi–Cu = 39.1–44.7 cm−1, and −JNi–Ni = 26.3–26.6 cm−1) leads to a non-compensation of the ground spin state for the tetranuclear MIIM′II3 star units [SA = SB = 3SM′−SM = 1 (1 and 2), 1/2 (3 and 4), and 2 (5 and 6)]. Within the binuclear MII2meso-helicate cores of 1–4, a moderate to weak antiferromagnetic coupling between the MII ions (−J′Cu–Cu = 28.0–48.0 cm−1 and −J′Ni–Ni = 0.16–0.97 cm−1) is mediated by the triple m-phenylenediamidate bridge to give a ground spin singlet (S = SA−SB = 0) state for the octanuclear MII2CuII6 molecule. Instead, a weak ferromagnetic coupling between the NiII ions (J′Ni–Ni = 2.07–3.06 cm−1) operates in the binuclear NiII2meso-helicate core of 5 and 6 leading thus to a ground spin nonet (S = SA + SB = 4) state for the octanuclear NiII8 molecule. Dc magnetization data for 5 reveal a small but non-negligible axial magnetic anisotropy (D = −0.23 cm−1) of the S = 4 NiII8 ground state with an estimated value of the energy barrier for magnetization reversal of 3.7 cm−1 (U = −DS2). Ac magnetic susceptibility data for 5 show an unusual slow magnetic relaxation behaviour at low temperatures which is typical of “cluster glasses”. The temperature dependence of the relaxation time for 5 has been interpreted on the basis of the Vogel–Fulcher law for weakly interacting clusters, with values of 2.5 K, 1.4 × 10−6 s, and 4.0 cm−1 for the intermolecular interaction parameter (T0), the pre-exponential factor (τ0), and the effective energy barrier (Ueff), respectively.
式为 Na2[Cu2(mpba)3][Cu(Me5dien)]6}(ClO4)6·12H2O (1), Na2[Cu2(Mempba)3][Cu(Me5dien)] 的同金属和异金属八核配合物6}(ClO4)6·12H2O (2), Na2[Ni2(mpba)3][Cu(Me5dien)]6}(ClO4)6·12H2O (3), Na2[Ni2(Mempba)3][Cu (Me5dien)]6}(ClO4)6·9H2O (4)、[Ni2(mpba)3][Ni(dipn)(H2O)]6}(ClO4)4·12.5H2O (5) 和 [Ni2 (Mempba)3][Ni(dipn)(H2O)]6}(ClO4)4·12H2O (6) [mpba = 1,3-亚苯基双(草酸酯), Mempba = 4-甲基-1,3-亚苯基双(草酸酯) ),Me5dien = N,N,N',N'',N''-五甲基二亚乙基三胺,dipn = 二亚丙基三胺]通过“配合物作为配体/配合物作为金属”策略合成。 1、3和5的单晶X射线衍射分析显示阳离子MII2M'II6实体(M,M'= Cu和Ni)具有整体双星结构,由两个oxamato桥联的MIIM'组成II3 星形单元通过两个中心金属原子之间的三个间苯二酰胺桥连接,形成内消旋型双核金属隐配体核心。通过“四聚体二聚体”模型分析了 2-300 K 温度范围内 1-6 的直流磁化率数据 [H = −J(S1A·S3A + S1A·S4A + S1A·S5A + S2B·S6B) + S2B·S7B + S2B·S8B) −J′S1A·S2B,其中 S1A = S2B = SM 且 S3A = S4A = S5A = S6B = S7B = S8B = SM′]。 MII 和 M'II 离子之间通过 1-6 的草酸盐桥产生中度至强的反铁磁耦合(−JCu–Cu = 52.0–57.0 cm−1,−JNi–Cu = 39.1–44.7 cm−1,−JNi –Ni = 26.3–26.6 cm−1) 导致四核 MIIM′II3 星单元的基自旋态不补偿 [SA = SB = 3SM′−SM = 1 (1 和 2), 1/2 ( 3和4)和2(5和6)]。在 1-4 的双核 MII2 介观螺旋核内,MII 离子之间存在中度至弱的反铁磁耦合(−J′Cu–Cu = 28.0–48.0 cm−1 和 −J′Ni–Ni = 0.16–0.97 cm−1 )由三重间苯二胺桥介导,为八核 MII2CuII6 分子提供地自旋单线态 (S = SA−SB = 0) 状态。相反,NiII 离子之间的弱铁磁耦合 (J′Ni–Ni = 2.07–3.06 cm−1) 在 5 和 6 的双核 NiII2 介观螺旋核心中运行,从而导致地自旋诺奈特 (S = SA + SB = 4)八核NiIII8分子的状态。 5 的直流磁化数据揭示了 S = 4 NiIII8 基态的小但不可忽略的轴向磁各向异性 (D = -0.23 cm−1),磁化反转的能量势垒估计值为 3.7 cm−1 (U =−DS2)。 5 的交流磁化率数据显示出低温下不寻常的慢磁弛豫行为,这是“簇玻璃”的典型特征。 5 的弛豫时间的温度依赖性已根据弱相互作用团簇的 Vogel-Fulcher 定律进行了解释,分子间相互作用参数值为 2.5 K、1.4 × 10−6 s 和 4.0 cm−1 ( T0)、指前因子 (τ0) 和有效能垒 (Ueff)。