Astrophysical line diagnosis requires nonlinear dynamical atomic modeling.

Natalia S Oreshkina1, Stefano M Cavaletto1, Christoph H Keitel1

  • 1Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany.

Physical Review Letters
|October 18, 2014
PubMed
Summary

Researchers calculated line intensities and oscillator strengths for neonlike iron ions. Nonlinear dynamical effects, not just electron correlation, may resolve discrepancies in astrophysical spectral line analysis.

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