corner
corner

Phys. Rev. B 75, 195121 (2007) [11 pages]

Spectral and Fermi surface properties from Wannier interpolation

Download: PDF (526 kB) Buy this article Export: BibTeX or EndNote (RIS)

Jonathan R. Yates1,2, Xinjie Wang3, David Vanderbilt3, and Ivo Souza1,2
1Department of Physics, University of California, Berkeley, California 94720, USA
2Materials Science Division, Lawrence Berkeley Laboratory, Berkeley, California 94720, USA
3Department of Physics and Astronomy, Rutgers University, Piscataway, New Jersey 08854-8019, USA

Received 23 February 2007; revised 27 April 2007; published 21 May 2007

We present an efficient first-principles approach for calculating Fermi surface averages and spectral properties of solids, and use it to compute the low-field Hall coefficient of several cubic metals and the magnetic circular dichroism of iron. The first step is to perform a conventional first-principles calculation and store the low-lying Bloch functions evaluated on a uniform grid of k points in the Brillouin zone. We then map those states onto a set of maximally localized Wannier functions, and evaluate the matrix elements of the Hamiltonian and the other needed operators between the Wannier orbitals, thus setting up an “exact tight-binding model.” In this compact representation the k-space quantities are evaluated inexpensively using a generalized Slater-Koster interpolation. Owing to the strong localization of the Wannier orbitals in real space, the smoothness and accuracy of the k-space interpolation increases rapidly with the number of grid points originally used to construct the Wannier functions. This allows k-space integrals to be performed with ab initio accuracy at low cost. In the Wannier representation, band gradients, effective masses, and other k derivatives needed for transport and optical coefficients can be evaluated analytically, producing numerically stable results even at band crossings and near weak avoided crossings.

© 2007 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevB.75.195121
DOI:
10.1103/PhysRevB.75.195121
PACS:
71.15.Dx, 71.18.+y, 71.20.−b, 75.47.−m