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pdf, 9 MiB - Infoscience - EPFL

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6.13. CONCLUSION 171<br />

0.15<br />

C ij<br />

=<br />

0.10<br />

0.05<br />

0.00<br />

0.0<br />

0.2<br />

0.4<br />

0.6<br />

V 2<br />

Figure 6.22: Lanczos calculations of the current-current correlations for the two<br />

most distant links in a 8 copper lattice with 10 holes (Si<br />

z = 0). The correlations<br />

of the current operator increase strongly with V 2 .<br />

By applying the variational Monte Carlo procedure to the extended Hamiltonian<br />

containing both the parameters of the usual three-band Hubbard Hamiltonian<br />

and the correlated hopping term V 2 , we find a clear enhancement of the<br />

orbital currents when V 2 > 0.4. The currents become large when the doping is<br />

close to x ≈ 0.12. In the VMC frame, we find that the symmetry of the charge<br />

currents is still θ 2 like (Fig. 6.24). The current-current correlations in a small 8<br />

copper cluster were also calculated, and we find very strong correlations, though<br />

the symmetry in the small cluster is θ 1 like (see Fig. 6.22 and Fig. 6.24). The<br />

change of the orbital current pattern between the small 8 copper lattice and larger<br />

lattice suggests that the finite-size effects are too strong on cluster as small as<br />

8 coppers. Although it is difficult to extract a well defined current value in the<br />

Lanczos calculations, we show in Fig. 6.22 how the current correlations evolve<br />

when the correlated hopping term increases.<br />

6.13 Conclusion<br />

In this work we have considered several scenarii that are shedding light on the possibility<br />

for spontaneous time reversal symmetry breaking in Hubbard-like models.<br />

As a first step, we have considered a simple three-site ring with a pair of holes:<br />

this small model already shows that when the hopping integral t is positive, there<br />

is a natural trivial charge circulation. Indeed, further variational Monte Carlo<br />

and mean-field calculations show that for some particular choices of the sign of<br />

the hopping transfer integral within the three-band Hubbard model, orbital currents<br />

are strongly stabilized. When the choice of the hopping sign leads to 2<br />

triangles with positive hopping sign around each copper site, the resulting sym-

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