A highly optimized code for calculating atomic data at neutron star magnetic field strengths using a doubly self-consistent Hartree–Fock

A highly optimized code for calculating atomic data at neutron star magnetic field strengths using a doubly self-consistent Hartree–Fock–Roothaan method

Published:2012-07 Issue:7 Volume:183 Page:1502-1510
ISSN:0010-4655
Container-title:Computer Physics Communications
language:en
Short-container-title:Computer Physics Communications

Author:

Schimeczek C.,Engel D.,Wunner G.

Funder

bwGRiD

Publisher

Elsevier BV

Subject

General Physics and Astronomy,Hardware and Architecture

Reference28 articles.

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

2. Discovery of Absorption Features in the X-Ray Spectrum of an Isolated Neutron Star

3. Pulse Phase Variations of the X‐Ray Spectral Features in the Radio‐quiet Neutron Star 1E 1207−5209

4. A broad absorption feature in the X-ray spectrum of the isolated neutron star RBS1223 (1RXS J130848.6+212708)

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