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The SIESTA method for ab initio order-N materials simulation

José M Soler et al 2002 J. Phys.: Condens. Matter 14 2745-2779   doi: 10.1088/0953-8984/14/11/302  Help

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José M Soler1, Emilio Artacho2, Julian D Gale3, Alberto García4, Javier Junquera1,5, Pablo Ordejón6 and Daniel Sánchez-Portal7
1 Dep. de Física de la Materia Condensada, C-III, Universidad Autónoma de Madrid, E-28049 Madrid, Spain
2 Department of Earth Sciences, University of Cambridge, Downing St., Cambridge CB2 3EQ, UK
3 Department of Chemistry, Imperial College of Science, Technology and Medicine, South Kensington SW7 2AY, UK
4 Departamento de Física de la Materia Condensada, Universidad del País Vasco, Apt. 644, 48080 Bilbao, Spain
5 Institut de Physique, Bâtiment B5, Université de Liège, B-4000 Sart-Tilman, Belgium
6 Institut de Ciència de Materials de Barcelona, CSIC, Campus de la UAB, Bellaterra, 08193 Barcelona, Spain
7 Dep. de Física de Materiales and DIPC, Facultad de Química, UPV/EHU, Apt. 1072, 20080 Donostia, Spain

Abstract. We have developed and implemented a selfconsistent density functional method using standard norm-conserving pseudopotentials and a flexible, numerical linear combination of atomic orbitals basis set, which includes multiple-zeta and polarization orbitals. Exchange and correlation are treated with the local spin density or generalized gradient approximations. The basis functions and the electron density are projected on a real-space grid, in order to calculate the Hartree and exchange-correlation potentials and matrix elements, with a number of operations that scales linearly with the size of the system. We use a modified energy functional, whose minimization produces orthogonal wavefunctions and the same energy and density as the Kohn-Sham energy functional, without the need for an explicit orthogonalization. Additionally, using localized Wannier-like electron wavefunctions allows the computation time and memory required to minimize the energy to also scale linearly with the size of the system. Forces and stresses are also calculated efficiently and accurately, thus allowing structural relaxation and molecular dynamics simulations.

Print publication: Issue 11 (25 March 2002)
Received 12 November 2001, in final form 16 January 2002
Published 8 March 2002

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