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arXiv · 1003.3188

Spectral function of the Anderson impurity model at finite temperatures

Aldo Isidori·David Roosen·Lorenz Bartosch·Walter Hofstetter·Peter Kopietz
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Abstract

Using the functional renormalization group (FRG) and the numerical renormalization group (NRG), we calculate the spectral function of the Anderson impurity model at zero and finite temperatures. In our FRG scheme spin fluctuations are treated non-perturbatively via a suitable Hubbard-Stratonovich field, but vertex corrections are neglected. A comparison with our highly accurate NRG results shows that this FRG scheme gives a quantitatively good description of the spectral line-shape at zero and finite temperatures both in the weak and strong coupling regimes, although at zero temperature the FRG is not able to reproduce the known exponential narrowing of the Kondo resonance at strong coupling.

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Aldo Isidori, David Roosen, Lorenz Bartosch, Walter Hofstetter, Peter Kopietz. 2010-03-16. Spectral function of the Anderson impurity model at finite temperatures. https://doi.org/10.1103/physrevb.81.235120

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