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NCA is a self-consistent perturbation theory for the single-impurity Anderson model and is often a fast method to obtain results for this model and also within DMFT. However, NCA is known to violate Fermi liquid properties at temperatures much lower than the smallest energy scale of the problem and whenever charge excitations become important [37,39]. Hence, in some parameter ranges it fails to account for the proper low-energy physics and must therefore be applied with considerable care [39]
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NCA is a self-consistent perturbation theory for the single-impurity Anderson model and is often a fast method to obtain results for this model and also within DMFT. However, NCA is known to violate Fermi liquid properties at temperatures much lower than the smallest energy scale of the problem and whenever charge excitations become important [37,39]. Hence, in some parameter ranges it fails to account for the proper low-energy physics and must therefore be applied with considerable care [39].
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At present, QMC simulations of the DMFT equations are not feasible at the experimental temperature (80 K). We note, however, that no intrinsic temperature dependence was observed in the experiment [40], at least up to room temperature
-
At present, QMC simulations of the DMFT equations are not feasible at the experimental temperature (80 K). We note, however, that no intrinsic temperature dependence was observed in the experiment [40], at least up to room temperature.
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53
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0042960524
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In Figure 4, the distance between the lower Hubbard band and the chemical potential is seen to decrease with increasing U. Note, however, that the upper Hubbard band is also shifted to higher energies
-
In Figure 4, the distance between the lower Hubbard band and the chemical potential is seen to decrease with increasing U. Note, however, that the upper Hubbard band is also shifted to higher energies.
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54
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0042459441
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If one multiplies the IPT and NCA results of Figure 3 with the Fermi function and employs a broadening of 0.3 eV one obtains a spectrum where the lower Hubbard band is nearer to the Fermi energy and which has a less pronounced minimum or shoulder between Hubbard and quasi-particle band
-
If one multiplies the IPT and NCA results of Figure 3 with the Fermi function and employs a broadening of 0.3 eV one obtains a spectrum where the lower Hubbard band is nearer to the Fermi energy and which has a less pronounced minimum or shoulder between Hubbard and quasi-particle band.
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55
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