Orbital Currents in Extended Hubbard Models of High-Tc Cuprate Superconductors

Cédric Weber, Andreas Läuchli, Frédéric Mila, and Thierry Giamarchi
Phys. Rev. Lett. 102, 017005 – Published 8 January 2009

Abstract

Motivated by the recent report of broken time-reversal symmetry and zero momentum magnetic scattering in underdoped cuprates, we investigate under which circumstances orbital currents circulating inside a unit cell might be stabilized in extended Hubbard models that explicitly include oxygen orbitals. Using Gutzwiller projected variational wave functions that treat on an equal footing all instabilities, we show that orbital currents indeed develop on finite clusters and that they are stabilized in the thermodynamic limit if additional interactions, e.g., strong hybridization with apical oxygens, are included in the model.

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  • Received 27 March 2008

DOI:https://doi.org/10.1103/PhysRevLett.102.017005

©2009 American Physical Society

Authors & Affiliations

Cédric Weber1, Andreas Läuchli2, Frédéric Mila3, and Thierry Giamarchi4

  • 1Department of Physics and Astronomy, Rutgers University, Piscataway, New Jersey 08854, USA
  • 2Institut Romand de Recherche Numérique en Physique des Matériaux (IRRMA), CH-1015 Lausanne, Switzerland
  • 3Institute of Theoretical Physics, EPFL, CH-1015 Lausanne, Switzerland
  • 4DPMC-MaNEP, University of Geneva, 24 Quai Ernest-Ansermet, CH-1211 Geneva, Switzerland

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Issue

Vol. 102, Iss. 1 — 9 January 2009

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