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5 Hirsch-Fye quantum Monte Carlo method for ... - komet 337

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5.22 Nils Blümer<br />

1<br />

0.8<br />

0.6<br />

Z<br />

0.4<br />

0.2<br />

0<br />

0.25<br />

0.2<br />

0.15<br />

D<br />

0.1<br />

0.05<br />

0<br />

E<br />

0.4<br />

0.2<br />

0<br />

-0.2<br />

-0.4<br />

-0.6<br />

-0.8<br />

0 1 2 3 4 5 6<br />

U<br />

T=0.1<br />

E pot<br />

E tot<br />

E kin<br />

2OPT: T=0<br />

Fig. 13: Quasiparticle weightZ (discrete estimate), double occupancyD, and energy contributions<br />

<strong>for</strong> the 1-band Hubbard model on the Bethe lattice (bandwidthW = 4) at T = 0.1 in the<br />

paramagnetic phase. Crosses (connected with lines) denote QMC results <strong>for</strong>∆τ = 0.2, squares<br />

are <strong>for</strong> ∆τ = 0.125. For comparison, results of second order perturbation theory (2OPT) are<br />

shown <strong>for</strong> the total energy and the double occupancy <strong>for</strong>T = 0 (solid black lines).<br />

metal-insulator transition so that its interpretation as a quasiparticle weight breaks down. In<br />

contrast, the discrete version (41) always leads to positive Z and may there<strong>for</strong>e appear more<br />

physical. In any case, Z loses its theoretical foundation outside the Fermi liquid phase where<br />

it remains only a heuristic indicator of a metal-insulator transition. In the uppermost part of<br />

Fig. 13, Z is shown <strong>for</strong> the relatively high temperature T = 0.1. A rapid change of slopes<br />

indicates a transition or crossover near U ≈ 4.7.<br />

Energy<br />

Within the DMFT, the energy per lattice site is given as [1, 8]<br />

�<br />

E = lim<br />

η→0 +T<br />

n,σ<br />

� ∞<br />

e<br />

dǫ<br />

iωnη ǫρ(ǫ)<br />

iωn −ǫ−Σσ(iωn)<br />

−∞<br />

1 �<br />

+ T Σσ(iωn)Gσ(iωn). (42)<br />

2<br />

n,σ

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