1994
DOI: 10.1103/physreva.49.809
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Force field and potential due to the Fermi-Coulomb hole charge for nonspherical-density atoms

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Cited by 27 publications
(10 citation statements)
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“…The local one-electron potential (7) can be considered as the path-independent work done in moving an electron belonging to a system from infinity to the reference point r against the electric field created by the total charge and the Fermi-Coulomb hole charge and a correlation-kinetic field. That means we follow a simple electrostatic interpretation of effective potential given by Slamet et al (1994), Liu et al (1999) and Sen et al (2002). It allows us to avoid the functional derivation and to facilitate a computation of the inner-molecule/crystal forces.…”
Section: Methodsmentioning
confidence: 99%
“…The local one-electron potential (7) can be considered as the path-independent work done in moving an electron belonging to a system from infinity to the reference point r against the electric field created by the total charge and the Fermi-Coulomb hole charge and a correlation-kinetic field. That means we follow a simple electrostatic interpretation of effective potential given by Slamet et al (1994), Liu et al (1999) and Sen et al (2002). It allows us to avoid the functional derivation and to facilitate a computation of the inner-molecule/crystal forces.…”
Section: Methodsmentioning
confidence: 99%
“…Here 𝜇(𝒓) is the chemical potential, i.e., the path-independent work that needs to be done for moving any electron belonging to a system from infinity to a reference point against the kinetic force field and the static Coulomb force field corrected for exchange. 22,[32][33][34] Functional 𝐸 𝑘 [𝜌] describes the noninteracting kinetic energy of electrons. In one-determinant approximation, the latter can be presented as the sum of Pauli 𝐸 𝑃 [𝜌] and von Weizsäcker 𝐸 𝑊 [𝜌] kinetic energy functionals.…”
Section: 𝜇[𝜌(𝒓)] = 𝛿𝐸 𝑘 [𝜌(𝒓)] 𝛿𝜌(𝒓) + 𝜑 𝑒𝑚 (𝒓)mentioning
confidence: 99%
“…For spherically symmetric densities, as used in atomic sphere approximation (ASA) in LMTO-ASA, this E is curl free. For nonspherical charge densities, the solenoidal part of E is related to the difference in kinetic energies between the HF and the HS approaches [88] and the contribution is numerically insignificant [89]. The HS potential can directly be derived from Schrödinger equation [90].…”
Section: Orbital Based Exchange Correlationmentioning
confidence: 99%