Transport Coefficients of the Anderson Model via the Numerical Renormalization Group

Details Transport Coefficients of the Anderson Model via the Numerical Renormalization Group Transport Coefficients of the Anderson Model via the Numerical Renormalization Group

1993-10-14

arxiv.org/abs/cond-mat/9310032v1

J. Phys.: Cond. Matt. 6, 2519 (1994)

Physics

Condensed Matter

45 pages, RevTeX, 28 figures, available on request

Scientific paper

10.1088/0953-8984/6/13/013

The transport coefficients of the Anderson model are calculated by extending Wilson's NRG method to finite temperature Green's functions. Accurate results for the frequency and temperature dependence of the single--particle spectral densities and transport time $\tau(\omega,T)$ are obtained and used to extract the temperature dependence of the transport coefficients in the strong correlation limit. The low temperature anomalies in the resistivity, $\rho(T)$, thermopower, $S(T)$, thermal conductivity $\kappa(T)$ and Hall coefficient, $R_{H}(T)$, are discussed. All quantities exhibit the expected Fermi liquid behaviour at low temperature with power law dependecies on $T/T_{K}$ in very good agreement with analytic results based on Fermi liquid theory. Scattering of conduction electrons in higher, $l>0$, angular momentum channels is also considered and an expression is derived for the corresponding transport time and used to discuss the influence of non--resonant scattering on the transport properties.

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