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Generalized gradient approximation for the exchange-correlation hole of a many-electron system

Generalized gradient approximation for the exchange-correlation hole of a many-electron system We construct a generalized gradient approximation (GGA) for the density n xc ( r , r + u ) at position r + u of the exchange-correlation hole surrounding an electron at r , or more precisely for its system and spherical average 〈 n xc ( u )〉=(4π ) - 1 ∫ d Ω u N - 1 ∫ d 3 r n ( r ) n xc ( r , r + u ). Starting from the second-order density gradient expansion, which involves the local spin densities n ↑ ( r ), n ↓ ( r ) and their gradients ∇ n ↑ ( r ),∇ n ↓ ( r ), we cut off the spurious large- u contributions to restore those exact conditions on the hole that the local spin density (LSD) approximation respects. Our GGA hole recovers the Perdew-Wang 1991 and Perdew-Burke-Ernzerhof GGA’s for the exchange-correlation energy, which therefore respect the same powerful hole constraints as LSD. When applied to real systems, our hole model provides a more detailed test of these energy functionals, and also predicts the observable electron-electron structure factor. © 1996 The American Physical Society. http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png Physical Review B American Physical Society (APS)

Generalized gradient approximation for the exchange-correlation hole of a many-electron system

Physical Review B , Volume 54 (23) – Dec 15, 1996
7 pages

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References (15)

Publisher
American Physical Society (APS)
Copyright
Copyright © 1996 The American Physical Society
ISSN
1095-3795
DOI
10.1103/PhysRevB.54.16533
Publisher site
See Article on Publisher Site

Abstract

We construct a generalized gradient approximation (GGA) for the density n xc ( r , r + u ) at position r + u of the exchange-correlation hole surrounding an electron at r , or more precisely for its system and spherical average 〈 n xc ( u )〉=(4π ) - 1 ∫ d Ω u N - 1 ∫ d 3 r n ( r ) n xc ( r , r + u ). Starting from the second-order density gradient expansion, which involves the local spin densities n ↑ ( r ), n ↓ ( r ) and their gradients ∇ n ↑ ( r ),∇ n ↓ ( r ), we cut off the spurious large- u contributions to restore those exact conditions on the hole that the local spin density (LSD) approximation respects. Our GGA hole recovers the Perdew-Wang 1991 and Perdew-Burke-Ernzerhof GGA’s for the exchange-correlation energy, which therefore respect the same powerful hole constraints as LSD. When applied to real systems, our hole model provides a more detailed test of these energy functionals, and also predicts the observable electron-electron structure factor. © 1996 The American Physical Society.

Journal

Physical Review BAmerican Physical Society (APS)

Published: Dec 15, 1996

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