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Phys. Rev. B 73, 224513 (2006) [12 pages]

Low-energy physical properties of high-Tc superconducting Cu oxides: A comparison between the resonating valence bond and experiments

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Kai-Yu Yang1, C. T. Shih2, C. P. Chou3, S. M. Huang3, T. K. Lee3, T. Xiang4, and F. C. Zhang1,5
1Centre of Theoretical and Computational Physics and Department of Physics, The University of Hong Kong, Hong Kong
2Department of Physics, Tunghai University, Taichung, Taiwan
3Institute of Physics, Academia Sinica, Taipei, Taiwan
4Institute of Theoretical Physics and Interdisciplinary Center of Theoretical Studies, Chinese Academy of Sciences, Beijing, China
5Department of Physics, University of Cincinnati, Cincinnati, Ohio 45221, USA

Received 16 March 2006; published 16 June 2006

In a recent review by Anderson and co-workers, it was pointed out that an early resonating valence bond (RVB) theory is able to explain a number of unusual properties of high-temperature superconducting (SC) Cu oxides. Here we extend previous calculations to study more systematically the low-energy physical properties of the plain vanilla d-wave RVB state, and to compare the results with the available experiments. We use a renormalized mean-field theory combined with variational Monte Carlo and power Lanczos methods to study the RVB state of an extended t-J model in a square lattice with parameters suitable for the hole-doped Cu oxides. The physical observable quantities we study include the specific heat, the linear residual thermal conductivity, the in-plane magnetic penetration depth, the quasiparticle energy at the antinode (π,0), the superconducting energy gap, the quasiparticle spectra, and the Drude weights. The traits of nodes (including kF, the Fermi velocity vF, and the velocity along Fermi surface v2), and the SC order parameter are studied. Comparisons of the theory and the experiments in cuprates show an overall qualitative agreement, especially on their doping dependences.

© 2006 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevB.73.224513
DOI:
10.1103/PhysRevB.73.224513
PACS:
74.20.Fg, 74.72.−h, 71.10.−w