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Phys. Rev. B 67, 064105 (2003) [15 pages]

Ab initio approach for high-pressure systems with application to high-pressure phases of boron:  Perturbative momentum-space potentials

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D. E. Segall*
Department of Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139

T. A. Arias
Laboratory of Atomic and Solid State Physics, Cornell University, Ithaca, New York 14853

See Also: Publisher's Note

Received 29 July 2002; revised 15 October 2002; published 24 February 2003; publisher error corrected 28 February 2003

Through the use of perturbation theory, in this work we develop a method which allows for a substantial reduction in the size of the plane-wave basis used in density-functional calculations. This method may be used for both pseudopotentials and all-electron calculations and is particularly beneficial in the latter case. In all cases, the approach has the advantage of allowing accurate predictions of transferability errors for any environment. Finally, this method can be easily implemented into conjugate-gradient techniques, and it is therefore computationally efficient. In this work, we apply this method to study high-pressure phases of boron. We find that boron undergoes a phase transition from the α12-B structure to the αga-B structure, both of which are semiconducting. The αga-B structure has lower energy than traditional monoatomic structures, which supports the assertion that the metallic, and hence superconducting phase, for boron is much more complicated than a simple monoatomic crystal.

© 2003 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevB.67.064105
DOI:
10.1103/PhysRevB.67.064105
PACS:
71.15.Ap, 61.50.Ks

*Present address: Department of Applied Physics, California Institute of Technology, Pasadena, California 91125.

See Also

Publisher's Note: D. E. Segall and T. A. Arias, Publisher’s Note: Ab initio approach for high-pressure systems with application to high-pressure phases of boron: Perturbative momentum-space potentials [Phys. Rev. B 67, 064105 (2003)], Phys. Rev. B 67, 069901 (2003).