Spectrum of neutral helium in strong magnetic fields

Matthew D. Jones, Gerardo Ortiz, and David M. Ceperley
Phys. Rev. A 59, 2875 – Published 1 April 1999
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Abstract

We present extensive and accurate calculations for the excited-state spectrum of spin-polarized neutral helium in a range of magnetic field strengths up to 1012G. Of considerable interest to models of magnetic white dwarf stellar atmospheres, we also present results for the dipole strengths of the low-lying transitions among these states. Our methods rely on a systematically saturated basis set approach to solving the Hartree-Fock self-consistent field equations, combined with an “exact” stochastic method to estimate the residual basis set truncation error and electron correlation effects. We also discuss the applicability of the adiabatic approximation to strongly magnetized multielectron atoms.

  • Received 10 November 1998

DOI:https://doi.org/10.1103/PhysRevA.59.2875

©1999 American Physical Society

Authors & Affiliations

Matthew D. Jones and Gerardo Ortiz

  • Theoretical Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545

David M. Ceperley

  • Department of Physics and National Center for Supercomputing Applications, University of Illinois at Urbana–Champaign 1110 West Green Street, Urbana, Illinois 61801

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Issue

Vol. 59, Iss. 4 — April 1999

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