Origin of Hund’s multiplicity rule in singly excited helium: Existence of a conjugate Fermi hole in the lower spin state

Tokuei Sako, Josef Paldus, Atsushi Ichimura, and Geerd H. F. Diercksen
Phys. Rev. A 83, 032511 – Published 28 March 2011

Abstract

The origin of Hund’s multiplicity rule in the low-lying excited states of the helium atom has been studied by considering the two-dimensional helium atom. The internal part of the full configuration interaction wave functions for the (2s) and (2p) singlet-triplet pairs of states has been extracted and visualized in the three-dimensional internal space (r1,r2, ϕ). The internal wave function of the singlet states without electron repulsion has a significant probability around the origin of the internal space while the corresponding probability of the triplet wave function is negligible in this region due to the presence of a Fermi hole. The electron-electron repulsion potential has been visualized also in the internal space. It manifests itself by three striking poles penetrating exactly into the spatial region defined by the Fermi hole. Because of the existence of these strong potential poles in the vicinity of the Fermi hole a major part of the singlet probability migrates out of this region. In contrast, the corresponding triplet wave function is less affected by these poles due to the presence of the Fermi hole. The singlet probability is shown to migrate from its original region close to the origin to a region far away where either r1 or r2 are large. This results in a more diffuse electron density distribution and a smaller electron repulsion energy of the singlet state than of the corresponding triplet state. The mechanism of the evolution of the singlet probability toward the region of large ri (i =1, 2) in the presence of the electron repulsion potential has been rationalized on the basis of a new concept called conjugateFermihole.

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  • Received 2 January 2011

DOI:https://doi.org/10.1103/PhysRevA.83.032511

©2011 American Physical Society

Authors & Affiliations

Tokuei Sako*

  • Laboratory of Physics, College of Science and Technology, Nihon University, 7-24-1 Narashinodai, Funabashi, 274-8501 Chiba, Japan

Josef Paldus

  • Department of Applied Mathematics, University of Waterloo, Waterloo, Ontario N2L 3G1, Canada

Atsushi Ichimura

  • Institute of Space and Astronautical Science, JAXA, Sagamihara 229-8510, Japan

Geerd H. F. Diercksen§

  • Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, D-85741 Garching, Germany

  • *sako@phys.ge.cst.nihon-u.ac.jp; http://www.phys.ge.cst.nihon-u.ac.jp/∼sako/
  • paldus@uwaterloo.ca; http://www.math.uwaterloo.ca/∼paldus/
  • ichimura@isas.jaxa.jp
  • §ghd@mpa-garching.mpg.de; http://www.mpa-garching.mpg.de/mol-physics/index.shtml

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Vol. 83, Iss. 3 — March 2011

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