Self-energy method for time-dependent spectral functions of the Anderson impurity model within the time-dependent numerical renormalization group approach
H. T. M. Nghiem, T. A. Costi

TL;DR
This paper extends the self-energy method to time-dependent spectral functions in the Anderson impurity model, improving accuracy and providing clear insights into spectral evolution over time within the time-dependent NRG framework.
Contribution
It generalizes the self-energy approach to time-dependent problems in quantum impurity models using the equation of motion method.
Findings
Improved accuracy in time-dependent spectral function calculations.
Closed-form expressions enable clear visualization of spectral evolution.
Potential applicability to other quantum impurity solvers.
Abstract
The self-energy method for quantum impurity models expresses the correlation part of the self-energy in terms of the ratio of two Green's functions and allows for a more accurate calculation of equilibrium spectral functions than is possible directly from the one-particle Green's function [Bulla et al., J. Phys.: Condens. Matter 10, 8365 (1998)], for example, within the numerical renormalization group method. In addition, the self-energy itself is a central quantity required in the dynamical mean field theory of strongly correlated lattice models. Here, we show how to generalize the self-energy method to the time-dependent situation for the prototype model of strong correlations, the Anderson impurity model. We use the equation of motion method to obtain closed expressions for the local Green's function in terms of a time-dependent correlation self-energy, with the latter being given as…
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