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Multiorbital Hubbard model in infinite dimensions: Quantum Monte Carlo calculation

J. E. Han, M. Jarrell, and D. L. Cox
Phys. Rev. B 58, R4199(R) – Published 15 August 1998
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Abstract

Using the quantum Monte Carlo technique we compute thermodynamics and spectra for the orbitally degenerate Hubbard model in infinite spatial dimensions. With increasing orbital degeneracy we find in the one-particle spectra broader Hubbard bands (consistent with increased kinetic energy), a narrowing Mott gap, and increasing quasiparticle spectral weight. Hund’s rule exchange coupling decreases the critical on-site Coulomb energy for the Mott transition. The metallic regime resistivity for twofold degeneracy is quadratic in temperature at low temperatures.

  • Received 1 April 1998

DOI:https://doi.org/10.1103/PhysRevB.58.R4199

©1998 American Physical Society

Authors & Affiliations

J. E. Han

  • Max-Planck Institut für Festköperforschung, Heisenbergstrasse 1, D-70569 Stuttgart, Germany

M. Jarrell

  • Department of Physics, University of Cincinnati, Cincinnati, Ohio 45221

D. L. Cox

  • Department of Physics, University of California, Davis, California 95616

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Vol. 58, Iss. 8 — 15 August 1998

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