SCF Relativistic Hartree–Fock Calculations on the Superheavy Elements 118–131

The energies of a number of configurations of the elements with atomic numbers 118–131 were computed by means of the relativistic Hartree–Fock method to establish the probable ground states. The series of elements beginning at 121 differs markedly from the lanthanide and actinide series because spin...

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Veröffentlicht in:J. Chem. Phys. 53: 2397-2406(15 Sep 1970) 1970-01, Vol.53 (6), p.2397-2406
Hauptverfasser: Mann, Joseph B., Waber, James T.
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container_issue 6
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container_title J. Chem. Phys. 53: 2397-2406(15 Sep 1970)
container_volume 53
creator Mann, Joseph B.
Waber, James T.
description The energies of a number of configurations of the elements with atomic numbers 118–131 were computed by means of the relativistic Hartree–Fock method to establish the probable ground states. The series of elements beginning at 121 differs markedly from the lanthanide and actinide series because spinp–orbit and direct relativistic effects cause the 8p1/2 electron states to be partially filled before the 7d3/2 states. The inner shell of 5g electrons begins to fill at element 125. The Breit magnetic interaction energy is calculated by a perturbation method; an approximate correlation energy correction is included. Isotopic mass effects on the atom total energy and on the electron eigenvalues are discussed.
doi_str_mv 10.1063/1.1674338
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Mex</creatorcontrib><description>The energies of a number of configurations of the elements with atomic numbers 118–131 were computed by means of the relativistic Hartree–Fock method to establish the probable ground states. The series of elements beginning at 121 differs markedly from the lanthanide and actinide series because spinp–orbit and direct relativistic effects cause the 8p1/2 electron states to be partially filled before the 7d3/2 states. The inner shell of 5g electrons begins to fill at element 125. The Breit magnetic interaction energy is calculated by a perturbation method; an approximate correlation energy correction is included. 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Phys. 53: 2397-2406(15 Sep 1970)</title><description>The energies of a number of configurations of the elements with atomic numbers 118–131 were computed by means of the relativistic Hartree–Fock method to establish the probable ground states. The series of elements beginning at 121 differs markedly from the lanthanide and actinide series because spinp–orbit and direct relativistic effects cause the 8p1/2 electron states to be partially filled before the 7d3/2 states. The inner shell of 5g electrons begins to fill at element 125. The Breit magnetic interaction energy is calculated by a perturbation method; an approximate correlation energy correction is included. 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The series of elements beginning at 121 differs markedly from the lanthanide and actinide series because spinp–orbit and direct relativistic effects cause the 8p1/2 electron states to be partially filled before the 7d3/2 states. The inner shell of 5g electrons begins to fill at element 125. The Breit magnetic interaction energy is calculated by a perturbation method; an approximate correlation energy correction is included. Isotopic mass effects on the atom total energy and on the electron eigenvalues are discussed.</abstract><doi>10.1063/1.1674338</doi><tpages>10</tpages></addata></record>
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subjects ATOMIC MODELS
CORRELATION ENERGY
ENERGY
ENERGY LEVELS
HARTREE- FOCK METHOD
N32250 -Physics-Atomic & Molecular Physics-Atomic Theory
ORBITS
RELATIVITY THEORY
SELF-CONSISTENT FIELD
TRANS 104 ELEMENTS
TRANSACTINIDE ELEMENTS/energy levels of superheavy, having Z = 118 to 131, self-consistent-field relativistic Hartree-Fock calculations of
title SCF Relativistic Hartree–Fock Calculations on the Superheavy Elements 118–131
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