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Alternatives to the Broken Symmetry Approach

Dalam dokumen Magnetic Interactions in Molecules and Solids (Halaman 148-152)

4.3 Accurate Computational Models

4.3.5 Alternatives to the Broken Symmetry Approach

J= 2(EBS−EHS)

Smax(Smax+1) (4.87)

which is the generalized form of Eq.4.69. This expression is also used in DFT when the BS determinant is considered to be a good representation of the singlet (or lowest spin) state as proposed by Ruiz and co-workers [6, 19, 22]. These authors often replace the denominator by 2(2S1S2+S2)withS2 S1 andS1+S2 = Smax to reflect situations with unequal spin moments on the two magnetic centers.

4.10 Calculate the expectation value ofSˆ2forΦ1 = |φ1φ2φ3φ4|in the zero overlap limit:φijij.

4.3 Accurate Computational Models 137 symmetry (as in atomic multiplets or ligand-field states in coordination complexes) but due toaccidental(near-)degeneracies. This extended approach was named the restricted ensemble Kohn–Sham (REKS) method [23,24]. An optimal set of Kohn–

Sham orbitals and occupation numbers is obtained by a minimization procedure that always maintains the spin and spatial symmetry of theN-electron state under study.

The approach has been used to calculate the coupling of two localized spin moments in binuclear transition metal complexes and the singlet-triplet splitting in biradical systems, such as twisted ethylene. Rather reasonable values of the magnetic coupling parameters were obtained. In general, the couplings are slightly too small, which may be attributed to the lack of spin polarization. An important advantage of the method is the fact that geometries can be optimized for open-shell singlet states within the DFT framework.

Spin-flip time-dependent DFTThe energy differences of the spin states involved in the magnetic interaction of two (or more) spin moments can be seen to some extent as vertical excitation energies, and hence, time-dependent DFT (or other lin- ear response methods as equation of motions coupled cluster [25]) could in principle be used to determine the magnetic interaction between two spin moments. However, the standard implementation of TD-DFT only considers single,spin-conservingexci- tations, which prevents accounting for the multideterminantal character of the states with low-spin coupling [26]. Figure4.12shows the five determinants that are essen- tial to describe the magnetic coupling in a two-electron/two-orbital problem. Using determinantΦ12orΦ3as reference will not generate all five determinants in stan- dard TD-DFT, whileΦ4andΦ5lead to the same spin contamination problems as in the BS approach discussed above. The spin-flip formalism (originally developed in the framework of Hartree–Fock and coupled cluster, and later implemented for TD-DFT) offers an interesting solution to this shortcoming. The determinant with maximumMS-value is taken as reference (Φ1in Fig.4.12) and all single excited deter- minants involving one spin-flip are generated from this. Within the space of the two- electron/two-orbital problem, this procedure generates the determinantsΦ2. . . Φ5 of Fig.4.12, and hence, gives access to the energy of the open-shell singlet within the TD-DFT framework without spin-contamination problems.

Constrained DFTThe basic shortcomings of the BS approach can be summarized in two points. In the first place, the spin contamination, or the impossibility to rep- resent the low-spin states with a single Kohn–Sham determinant. The second point is the fact that nearly all todays functionals tend to overestimate the delocalization of the spin density and overestimate the antiferromagnetic character of the coupling.

1 2 3 4 5

Fig. 4.12 The reference determinantΦ1and the four spin-flip determinants (Φ2. . . Φ5) generated in SF-TDDFT with a two-electron/two-orbital target space

Constrained DFT (C-DFT) remedies, at least partially, the latter by putting restric- tions on the spatial distributions of theαandβelectrons [27]. Two fragmentspand q are defined such that both include one magnetic center and the atoms around it.

Subsequently, the density is optimized under the restrictions thatNαp−Nβp = MSp andNαq−Nβq =MSq, whereNα,βp,q are the summed spin populations of the atoms in the fragments and MSp,qthe prefixed excess ofαorβ electrons in each fragment.

C-DFT results in less delocalized spin densities and therefore, in general, to smaller interaction parameters.

Problems

4.1 A master student wants to study the energy splitting ES −ET in a planar [Cu2F6]2−model system, since experimental studies of similar di Cl-bridged CuII dimers suggested that ES−ET depends strongly on the Cu–Cl–Cu angleθ. She performs RHF calculations on the triplet state in order to predictES−ET with the HTH model. She produces a Table of results, where thegeradeandungeradeopen shell orbitals are denoted 1 and 2, respectively.

θ J11+J222J12[K]K12[Eh]ε1ε2[Eh]

85 24 0.4324 0.0078

90 20 0.4376 0.0025

95 22 0.4419 0.0034

100 26 0.4456 0.0094

105 32 0.4483 0.0150

ComputeJ (in K) forθ = 85. . .105using the HTH model. Do you observe a strong dependence of the coupling on the angle? Can the same conclusions be drawn when only considering the orbital energies?

4.2 Quantifying the counter-complementarity effect. Standard optimization of the molecular orbitals of a magnetic complex with two magnetic centers bridged by two different ligands normally leads to magnetic orbitals with contributions on both ligands (as ϕ5 and ϕ6 in Fig.4.9). This makes it very hard to quantify the counter-complementary effect of the two ligands. Design a computational strategy to determine quantitatively the reduction of the magnetic coupling through ligand 1 by the counter-complementary effect of ligand 2. Hint: Many quantum chemical programs can divide the whole system into fragments.

4.3 Broken symmetry approach. The magnetic coupling of three binuclear TM complexes has been studied with DFT. The following results were obtained for the HS and BS determinants. (a) Calculate the magnetic coupling parameterJwith the Yamaguchi equation (Eq.4.85) and compare the outcomes to the alternative relations of Noodleman (Eq.4.86) and Ruiz (Eq.4.87).

Problems 139

TM Energy [Eh] ˆS2

ΦHS ΦBS ΦHS ΦBS

Cu2+ 4061.74359204061.7442381 2.0035 0.9957 Ni2+ 3797.47424983797.4767694 6.0083 1.9931 Mn2+3082.75862973082.7630415 30.0086 4.9936

(b) CalculateJin the Cu complex combining Eqs.4.67and4.78usingραβis 0.6864 and 0.6757 for HS and BS, respectively.

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Towards a Quantitative Understanding

Abstract Taking a binuclear copper complex as model system, the isotropic mag- netic coupling is decomposed into different contributions. Perturbative expressions of the main contributions are derived and illustrated with numerical examples. An effective Hamiltonian is constructed that incorporates all important electron corre- lation effects and establishes a connection between the complex N-electron wave functions and the simpler qualitative methods discussed in the previous chapter.

Subsequently an outline is given of the analysis of the coupling with a single deter- minant approach and the biquadratic and four-center interactions are decomposed.

The chapter closes with the recently proposed method to extract DFT estimates for these complex interactions.

Dalam dokumen Magnetic Interactions in Molecules and Solids (Halaman 148-152)