A fast parallel code for calculating energies and oscillator strengths of many-electron atoms at neutron star magnetic field strengths in adiabatic approximation

DOI10.1016/j.cpc.2008.09.008zbMath1198.85003OpenAlexW2171549382MaRDI QIDQ603410

M. Klews, D. Engel, Günter Wunner

Publication date: 6 November 2010

Published in: Computer Physics Communications (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/j.cpc.2008.09.008

zbMATH Keywords

adiabatic approximationatomic dataneutron star magnetic fields\texttt{HFFEM}

Mathematics Subject Classification ID

Computational methods for problems pertaining to astronomy and astrophysics (85-08) Software, source code, etc. for problems pertaining to astronomy and astrophysics (85-04)

Related Items (2)

Multi-electron systems in strong magnetic fields. II: A fixed-phase diffusion quantum Monte Carlo application based on trial functions from a Hartree-Fock-Roothaan method ⋮ Accurate finite element method for atomic calculations based on density functional theory and Hartree-Fock method

Uses Software

• HFFEM

Cites Work

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• A practical guide to splines
• Generalised meshes for quantum mechanical problems
• Package for Calculating with B-Splines
• Asymptotics of heavy atoms in high magnetic fields: I. Lowest landau band regions
• Finite Elements
• On the computation of the eigenproblems of hydrogen and helium in strong magnetic and electric fields with the sparse grid combination technique

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