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Self-assembled Transition Metal Coordination Frameworks of ...

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Copper(lI) complexes<br />

F1 = g",3B:S: + gl,B(BxSx +BySy)+ /1,3,1: + A,(s,1, +sy1,.) (1)<br />

The formation <strong>of</strong> a binuclear complex is connected with the antiferromagnetic<br />

coupling <strong>of</strong> two Cu(lI) ions, leading to a singlet ground state and an excited spin<br />

triplet state. The energy difference, 2J , between these states depends on the strength<br />

<strong>of</strong> the interaction. If the triplet state is thermally accessible (2J ~ kT~ 200—400 cm"),<br />

paramagnetism is observed and the EPR spectra could be satisfactorily described<br />

using the interactive spin Hamiltonian [32] for isolated Cu(ll) dimer (S =1),<br />

I51=g,BBs+1)Sf +E(sf —sj)-1% (2)<br />

Where D and E are the zero field splitting parameters.<br />

However, the present spectra all indicate the presence <strong>of</strong> two different Cu(Il)<br />

species and there are no characteristic features <strong>of</strong> transfer <strong>of</strong> any coupling between the<br />

two Cu(lI) centers by the bridging moiety connecting them in frozen DMF. So the<br />

spectra were simulated by considering with the presence <strong>of</strong> two noninteracting Cu(Il)<br />

d 9 groups using EasySpin [33] written in MATLAB to get accurate values <strong>of</strong> various<br />

EPR parameters g" , g L , A" (Cu), A i (Cu). The systems with the presence <strong>of</strong> two<br />

Cu(II) species, each species described by eqn. (3) [34], were considered; as the spectra<br />

all not showed typical coupled binuclear nature but show two monomeric axial<br />

species.<br />

Ho = p,1'§,gs+§A°'1 (3)<br />

Where the first term is the electron Zeeman interaction with the extemal<br />

magnetic field vector B0 and the second term represents the hyperfine interaction<br />

between the electron spin S and the nuclear spin I <strong>of</strong> the copper nucleus. The g<br />

and A matrices in eqn. (3) are assumed to be axially symmetric and coaxial, so that<br />

eqn. (3) is similar to eqn. (1). The various magnetic interaction parameters obtained<br />

by simulations are summarized in Table 4.4 for compounds 8 to 19.<br />

153

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