Transport and Optical Conductivity in the Hubbard Model: A High-Temperature Expansion Perspective

preprint2016arXivOpen access

Abstract

We derive analytical expressions for the spectral moments of the dynamical response functions of the Hubbard model using the high-temperature series expansion. We consider generic dimension dd as well as the infinite-dd limit, arbitrary electron density nn, and both finite and infinite repulsion UU. We use moment-reconstruction methods to obtain the one-electron spectral function, the self-energy, and the optical conductivity. They are all smooth functions at high-temperature and, at large-UU, they are featureless with characteristic widths of order the lattice hopping parameter tt. In the infinite-dd limit we compare the series expansion results with accurate numerical renormalization group and interaction expansion quantum Monte-Carlo results. We find excellent agreement down to surprisingly low temperatures, throughout most of the bad-metal regime which applies for T≳(1−n)DT \gtrsim (1-n)D, the Brinkman-Rice scale. The resistivity increases linearly in TT at high-temperature without saturation. This results from the 1/T1/T behaviour of the compressibility or kinetic energy, which play the role of the effective carrier number. In contrast, the scattering time (or diffusion constant) saturate at high-TT. We find that σ(n,T)≈(1−n)σ(n=0,T)σ(n,T) \approx (1-n)σ(n=0,T) to a very good approximation for all nn, with σ(n=0,T)∝t/Tσ(n=0,T)\propto t/T at high temperatures. The saturation at small nn occurs due to a compensation between the density-dependence of the effective number of carriers and that of the scattering time. The TT-dependence of the resistivity displays a knee-like feature which signals a cross-over to the intermediate-temperature regime where the diffusion constant (or scattering time) start increasing with decreasing TT. At high-temperatures, the thermopower obeys the Heikes formula, while the Wiedemann-Franz law is violated with the Lorenz number vanishing as 1/T21/T^2.

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