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Spectral functions of one-dimensional models of correlated electrons

Julien Favand, Stephan Haas, Karlo Penc, Frédéric Mila, and Elbio Dagotto
Phys. Rev. B 55, R4859(R) – Published 15 February 1997
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Abstract

Using the Ogata-Shiba wave function, the spectral functions of the one-dimensional infinite-U Hubbard model are calculated for various concentrations. It is shown that the ``shadow-band'' feature due to 2kF fluctuations becomes more intense close to half filling. Comparing these results with exact-diagonalization data obtained on finite clusters for the finite-U Hubbard model and for the t-J model, it is also shown that this feature remains well defined for physically reasonable values of the parameters (U/t≃10, J/t≃0.4). The ``shadow'' structure in the spectral functions should thus be observable in angle-resolved photoemission experiments for a variety of quasi-one-dimensional compounds.

  • Received 21 October 1996

DOI:https://doi.org/10.1103/PhysRevB.55.R4859

©1997 American Physical Society

Authors & Affiliations

Julien Favand

  • Laboratoire de Physique Quantique, UniversitéPaul Sabatier, 31062 Toulouse, France

Stephan Haas

  • Theoretische Physik, ETH-Hönggerberg, 8093 Zürich, Switzerland

Karlo Penc

  • Max-Planck-Institut für Physik komplexer Systeme, Bayreuther Strasse 40, 01187 Dresden, Germany

Frédéric Mila

  • Laboratoire de Physique Quantique, UniversitéPaul Sabatier, 31062 Toulouse, France

Elbio Dagotto

  • Department of Physics and National High Magnetic Field Laboratory, Florida State University, Tallahassee, Florida 32306

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Vol. 55, Iss. 8 — 15 February 1997

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